This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 26.2712 2461125.7712 13.62 17:34:43.04 +40:55:40.0
66.29394 31.30771 galactic Her Second-epoch detections are separated by 2.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1344183205823151104 | 17:34:40.49 +40:56:07.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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!
TCP 2026 03 26.2712* 17 34 43.04 +40 55 40.0 13.6 U Her 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
Gaia DR3 1344183205823151104,2461125.7712,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1344183205823151104 20260326.2712 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:34:43.04 +40:55:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2712 2461125.7712 13.86 17:50:38.63 +39:31:54.1
65.43810 28.04674 galactic Her Second-epoch detections are separated by 4.1" and 4.9 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 J267.6632+39.5311 | 17:50:38.63 +39:31:54.1 (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!
TCP 2026 03 26.2712* 17 50 38.63 +39 31 54.1 13.9 U Her 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
ATO J267.6632+39.5311,2461125.7712,13.86,0.05,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 J267.6632+39.5311 20260326.2712 13.86CV 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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:50:38.63 +39:31:54.1 ;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_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20_00sec_-10_00C_LIGHT_0507_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20_00sec_-14_90C_LIGHT_0374_fits__*pix.png resample_wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20_00sec_-10_00C_LIGHT_0506_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: 2461121.97388028 22.03.2026 11:22:13.256 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
First image: 2461121.97388028 22.03.2026 11:22:13.256 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Last image: 2461125.77153459 26.03.2026 06:30:50.589 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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): 11554
Objects passed selection criteria: 11528
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 9494.25
Average stars matched: 9267 (97.6064 %)
Memory usage VmPeak: 117932 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 Thu Mar 26 01:33:04 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461121.97388028 22.03.2026 11:22:13.256 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
First image: 2461121.97388028 22.03.2026 11:22:13.256 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Last image: 2461125.77153459 26.03.2026 06:30:50.589 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
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: 37 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): 73114
Objects passed selection criteria: 72972
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 61139.5
Average stars matched: 58987.5 (96.4802 %)
Memory usage VmPeak: 1991520 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 Thu Mar 26 01:34:24 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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
SExtractor catalog cache: saved Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat to cache
SExtractor catalog cache: saved Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461125.77096061
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits exists and is non-empty
Saving wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits to local_wcs_cache/
'wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits' -> 'local_wcs_cache/wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits'
wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits exists and is non-empty
Saving wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits to local_wcs_cache/
'wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits' -> 'local_wcs_cache/wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits'
wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits exists and is non-empty
Saving wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits to local_wcs_cache/
'wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits' -> 'local_wcs_cache/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits'
wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits exists and is non-empty
Saving wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits to local_wcs_cache/
'wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits' -> 'local_wcs_cache/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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 17:27:15.979 +38:00:06.67
Second-epoch image center 17:27:10.882 +37:59:36.92
Angular distance between the image centers 0.02 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 17:27:15.979 +38:00:06.67
Second-epoch image center 17:27:09.710 +37:59:11.46
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:27:10.882 +37:59:36.92
Second-epoch second image center 17:27:09.710 +37:59:11.46
Angular distance between the image centers 0.00805 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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits &> /tmp/tmp.B9bBuACD2J
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits &> /tmp/tmp.UmUBlE1ldT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits &> /tmp/tmp.gGww9NlpWH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits &> /tmp/tmp.hFvNp9WPlH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits and wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits and wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
Found non-empty wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits and wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
The reference image (wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits) and catalog (wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat) found
'wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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 7700 out of 15186 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.942581
a=0.000000 b=1.000000 c=22.942581
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
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:
2.1 pix Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
2.1 pix Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
2.5 pix fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
2.5 pix fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Limiting magnitude estimates:
15.5 mag. Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
15.5 mag. Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
14.6 mag. fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
14.6 mag. fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.B9bBuACD2J (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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits' -> 'wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WCS_IMAGE_NAME=wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WCS-calibrated image found: wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Checking if the catalog wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits alredy exist and is non-empty...
Catalog wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WCS catalog name: wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1129, passed=15186
Got 15186 stars (including 14036 good ones) from the SExtractor catalog wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
util/solve_plate_with_UCAC5 got 15186 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits -region wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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.UmUBlE1ldT (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/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits' -> 'wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WCS_IMAGE_NAME=wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WCS-calibrated image found: wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
Checking if the catalog wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits alredy exist and is non-empty...
Catalog wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WCS catalog name: wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1149, passed=15112
Got 15112 stars (including 13944 good ones) from the SExtractor catalog wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat
util/solve_plate_with_UCAC5 got 15112 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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: 0.31"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits -region wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.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.gGww9NlpWH (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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
WCS-calibrated image found: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
Checking if the catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
WCS catalog name: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=502, passed=8517
Got 8517 stars (including 8009 good ones) from the SExtractor catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 8517 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 954 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits -region wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.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.hFvNp9WPlH (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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Checking if the catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
WCS catalog name: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, passed=8519
Got 8519 stars (including 8010 good ones) from the SExtractor catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 8519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 956 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits -region wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits'
Saving fully-calibrated image wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits'
Saving fully-calibrated image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits'
Saving fully-calibrated image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits'
Preparing the HTML report for the field Her-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Her-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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
SExtractor catalog cache: saved Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat to cache
SExtractor catalog cache: saved Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Creating symlink local_wcs_cache/wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
Creating symlink local_wcs_cache/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
Creating symlink local_wcs_cache/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits exists and is non-empty
wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits exists and is non-empty
wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits exists and is non-empty
wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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 17:27:15.979 +38:00:06.67
Second-epoch image center 17:27:10.882 +37:59:36.92
Angular distance between the image centers 0.02 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 17:27:15.979 +38:00:06.67
Second-epoch image center 17:27:09.710 +37:59:11.46
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:27:10.882 +37:59:36.92
Second-epoch second image center 17:27:09.710 +37:59:11.46
Angular distance between the image centers 0.00805 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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits &> /tmp/tmp.AqKqPLLPue
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits &> /tmp/tmp.II2reht5wx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits &> /tmp/tmp.Q98S2mONuW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits &> /tmp/tmp.Bea1ssQbGG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Calibrating the magnitude scale
Found non-empty wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits and wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits and wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
Found non-empty wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits and wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
The reference image (wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits) and catalog (wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat) found
'wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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 7730 out of 93479 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.817785
a=0.000000 b=1.000000 c=22.817785
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.68
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
1.9 pix Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
2.3 pix fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
2.3 pix fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Limiting magnitude estimates:
15.7 mag. Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
15.7 mag. Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
14.7 mag. fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
14.8 mag. fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.2 (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.AqKqPLLPue (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/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits' -> 'wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WCS_IMAGE_NAME=wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WCS-calibrated image found: wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Checking if the catalog wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits alredy exist and is non-empty...
Catalog wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
WCS catalog name: wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=6762, passed=93456
Got 93456 stars (including 86530 good ones) from the SExtractor catalog wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat
util/solve_plate_with_UCAC5 got 93456 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits -region wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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.II2reht5wx (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/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits' -> 'wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WCS_IMAGE_NAME=wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WCS-calibrated image found: wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
Checking if the catalog wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits alredy exist and is non-empty...
Catalog wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat corresponding to the image wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
WCS catalog name: wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=6884, passed=95010
Got 95010 stars (including 87966 good ones) from the SExtractor catalog wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat
util/solve_plate_with_UCAC5 got 95010 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits -region wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.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.Q98S2mONuW (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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
WCS-calibrated image found: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
Checking if the catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
WCS catalog name: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2507, passed=49926
Got 49926 stars (including 47359 good ones) from the SExtractor catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 49926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.47"
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_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits -region wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.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.Bea1ssQbGG (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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Checking if the catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat corresponding to the image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
WCS catalog name: wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2489, passed=50689
Got 50689 stars (including 48125 good ones) from the SExtractor catalog wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 50689 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits -region wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_Her-03-Q2b1x1_2026-03-22_06-22-13_20.00sec_-14.90C_LIGHT_0374.fits
Saving fully-calibrated image wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_Her-03-Q2b1x1_2026-03-22_06-23-18_20.00sec_-14.90C_LIGHT_0375.fits
Saving fully-calibrated image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-00_20.00sec_-10.00C_LIGHT_0506.fits
Saving fully-calibrated image wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.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_2026-03-26_CI_Her-03-Q2b1x1_013133_TTUQ2b1x1_22419_1s4fHFbY/wcs_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507.fits
Preparing the HTML report for the field Her-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out110768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out111502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111691.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110768_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 110768_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:11:32.55 +38:41:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 2.111 1341170333507874432 257.88565649976 +38.68589135403 14.4362 13.9224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110773_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 110773_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:29:45.40 +38:41:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.882 1343539441764592896 262.43931280567 +38.69135584875 14.5741 13.9762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110778_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 110778_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:19:58.79 +36:22:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 2.427 1336946426447071488 259.99489419929 +36.37903330907 14.3891 13.8633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110784_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 110784_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:52:39.22 +41:35:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.584 1345208947092332672 268.16321751064 +41.58985225821 14.1046 13.6411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110785_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 110785_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:56:54.66 +36:33:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.797 4609720302092921600 269.22714055326 +36.56185334493 13.6173 12.8842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110790_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 110790_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:46:11.78 +38:51:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.371 1342885369785841920 266.54861309680 +38.85752127311 13.7642 13.2630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111145_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111145_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:18:18.98 +38:50:35.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111193_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111193_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:51:10.67 +40:05:48.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111254_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111254_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:33:18.78 +41:14:41.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111256_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111256_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:51:17.52 +40:02:56.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111324_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111324_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:07:55.12 +35:57:13.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111339_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111339_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:48:00.08 +36:10:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111349_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111349_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:38:02.58 +34:58:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.382 4602596325738431232 264.51068529733 +34.98323065293 13.1437 12.4976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111374_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111374_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:51:14.60 +38:26:32.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111378_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111378_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:00:16.30 +34:21:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.752 1337938082857423872 255.06856164993 +34.35213162936 13.4930 13.0377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111396_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111396_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:47:49.83 +36:31:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.166 4608958615412769280 266.95659317399 +36.53085637456 13.5108 13.0046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111407_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111407_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:51:08.90 +40:03:14.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111416_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111416_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:46:58.51 +36:06:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.645 4608567666012429440 266.74451278274 +36.11266983272 13.4455 12.9833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111436_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111436_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:41:40.43 +35:22:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.682 4608625291590635648 265.41870251384 +35.37555114155 13.4536 12.9167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111480_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111480_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:27:40.49 +40:08:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.661 1346795645450239744 261.91811147482 +40.13626232715 13.8016 13.2242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111502_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
Preparing report for the candidate 111502_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111535_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111535_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:07:34.38 +33:49:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.984 1337721135467989504 256.89282484545 +33.83063205554 13.3089 12.1942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111551_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111551_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:54:05.44 +40:27:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.411 1344893627773630208 268.52146098799 +40.46129234464 14.0804 13.3095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111563_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111563_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:33:23.60 +36:46:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.775 1342377326693435136 263.35025864009 +36.77235837784 13.8592 13.0946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111593_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111593_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:42:29.92 +36:04:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.613 4608754862163754112 265.62579753878 +36.07922023561 13.8123 13.3975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111608_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111608_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:14:37.77 +42:12:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.442 1354152649550668416 258.65593022935 +42.20692886979 13.7408 13.1043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111621_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111621_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:17:05.98 +37:36:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.600 1340091854336318976 259.27439975851 +37.61320055062 13.7557 13.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111624_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111624_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:40:02.39 +35:08:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.634 4608595123740231296 265.01051251980 +35.14849737683 14.0897 13.5708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111626_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111626_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:05:27.37 +36:47:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.402 1339421942516993536 256.36394856815 +36.79311781981 13.9557 13.3197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111635_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111635_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:47:13.04 +38:19:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.203 1342788372244107008 266.80358816347 +38.31940344550 13.8854 13.2358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111647_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111647_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:20:47.87 +39:07:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.897 1340832993892587264 260.19970489847 +39.12196323566 13.5722 12.7451 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111691_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
Preparing report for the candidate 111691_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111692_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111692_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:29:26.79 +36:23:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.514 1336395227524180736 262.36152940948 +36.39060202791 14.3009 13.8417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111708_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111708_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:17:14.20 +36:22:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 3.828 1339866694970815232 259.30859054651 +36.36970675633 14.2087 13.7297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111721_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111721_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:43:43.70 +40:01:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.290 1343192683285266560 265.93222754938 +40.02318196777 14.0770 13.4575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111729_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111729_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:26:57.80 +37:51:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 4.494 1337482885042187008 261.73984236742 +37.85644508003 14.3985 13.8884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111767_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111767_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:28:33.81 +41:04:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.800 1347049632636163712 262.14022010512 +41.07296197332 14.1560 13.6367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111780_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111780_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:34:52.02 +34:04:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.386 4602427481983823872 263.71715710589 +34.07104067813 14.1610 13.6952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111783_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111783_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:41:41.75 +41:55:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.465 1345797903070829184 265.42446024070 +41.93131066947 14.6131 14.0804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111822_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111822_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks
**** FOUND 17:20:52.86 +36:29:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 3.511 1336971543415807744 260.21922034622 +36.49359920522 14.3991 13.8449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111911_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507
The candidate 111911_fd_Her-03-Q2b1x1_2026-03-26_01-30-50_20.00sec_-10.00C_LIGHT_0507 did not pass the final checks