This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.3074* 17 30 24.19 +17 54 48.0 12.7 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
UZ Her,2461125.8074,12.73,0.05,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
UZ Her 20260326.3074 12.73CV 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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:30:24.19 +17:54:48.0 ;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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20_00sec_-10_00C_LIGHT_0567_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20_00sec_-10_00C_LIGHT_0566_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20_00sec_-10_00C_LIGHT_0567_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20_00sec_-10_00C_LIGHT_0566_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.3074* 17 45 18.40 +17 15 32.9 13.4 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
V1427 Her,2461125.8074,13.37,0.05,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
V1427 Her 20260326.3074 13.37CV 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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:45:18.40 +17:15:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20_00sec_-10_00C_LIGHT_0567_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20_00sec_-10_00C_LIGHT_0566_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20_00sec_-10_00C_LIGHT_0567_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20_00sec_-15_00C_LIGHT_0595_fits__*pix.png resample_wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20_00sec_-10_00C_LIGHT_0566_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: 2461094.01803994 22.02.2026 12:25:48.651 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
First image: 2461094.01803994 22.02.2026 12:25:48.651 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Last image: 2461125.80869380 26.03.2026 07:24:21.144 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.03
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): 10976
Objects passed selection criteria: 10963
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 9998.25
Average stars matched: 9797.75 (97.9946 %)
Memory usage VmPeak: 119728 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 02:33:06 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: 2461094.01803994 22.02.2026 12:25:48.651 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
First image: 2461094.01803994 22.02.2026 12:25:48.651 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Last image: 2461125.80869380 26.03.2026 07:24:21.144 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 59 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): 88831
Objects passed selection criteria: 88679
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 80057.8
Average stars matched: 78001.8 (97.4319 %)
Memory usage VmPeak: 2472640 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 02:34:56 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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
SExtractor catalog cache: saved Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat to cache
SExtractor catalog cache: saved Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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: 2461125.80613300
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits exists and is non-empty
Saving wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits to local_wcs_cache/
'wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits' -> 'local_wcs_cache/wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits'
wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits exists and is non-empty
Saving wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits to local_wcs_cache/
'wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits' -> 'local_wcs_cache/wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits'
wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits exists and is non-empty
Saving wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits to local_wcs_cache/
'wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits' -> 'local_wcs_cache/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits'
wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits exists and is non-empty
Saving wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits to local_wcs_cache/
'wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits' -> 'local_wcs_cache/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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 17:46:40.862 +13:59:59.20
Second-epoch image center 17:46:39.496 +14:01:50.34
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:46:40.862 +13:59:59.20
Second-epoch image center 17:46:37.300 +14:02:03.77
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:46:39.496 +14:01:50.34
Second-epoch second image center 17:46:37.300 +14:02:03.77
Angular distance between the image centers 0.00963 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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits &> /tmp/tmp.v7ZknrHtIC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits &> /tmp/tmp.tOPMTPsy5n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits &> /tmp/tmp.obX8pe5ySa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits &> /tmp/tmp.zmKzUJ2OcC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits and wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits and wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
Found non-empty wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits and wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
The reference image (wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits) and catalog (wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat) found
'wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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 9514 out of 15011 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955879
a=0.000000 b=1.000000 c=22.955879
From vast_summary.log: estimated ref. image limiting mag.: -8.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.93
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.93
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
2.3 pix Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
2.7 pix fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
2.5 pix fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Limiting magnitude estimates:
14.9 mag. Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
14.9 mag. Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
14.4 mag. fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
14.4 mag. fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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.v7ZknrHtIC (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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits' -> 'wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WCS_IMAGE_NAME=wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WCS-calibrated image found: wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Checking if the catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits alredy exist and is non-empty...
Catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WCS catalog name: wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1150, passed=15011
Got 15011 stars (including 13841 good ones) from the SExtractor catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
util/solve_plate_with_UCAC5 got 15011 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 963 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits -region wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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.tOPMTPsy5n (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/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits' -> 'wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WCS_IMAGE_NAME=wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WCS-calibrated image found: wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
Checking if the catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits alredy exist and is non-empty...
Catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WCS catalog name: wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1096, passed=14607
Got 14607 stars (including 13492 good ones) from the SExtractor catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat
util/solve_plate_with_UCAC5 got 14607 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 963 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits -region wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.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.obX8pe5ySa (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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
WCS_IMAGE_NAME=wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
WCS-calibrated image found: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
Checking if the catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
WCS catalog name: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=594, passed=10488
Got 10488 stars (including 9884 good ones) from the SExtractor catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat
util/solve_plate_with_UCAC5 got 10488 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.60"
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_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits -region wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.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.zmKzUJ2OcC (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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
WCS_IMAGE_NAME=wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
WCS-calibrated image found: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Checking if the catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
WCS catalog name: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=657, passed=10474
Got 10474 stars (including 9810 good ones) from the SExtractor catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat
util/solve_plate_with_UCAC5 got 10474 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits -region wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits'
Saving fully-calibrated image wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits'
Saving fully-calibrated image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits'
Saving fully-calibrated image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits'
Preparing the HTML report for the field Oph-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20756.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20670_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 20670_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:35:40.08 +15:35:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20748_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 20748_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:48:12.01 +18:04:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20756_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 20756_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:51:54.63 +14:33:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.703 4500048204812795904 267.97788543565 +14.56329263844 12.1319 11.7177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Oph-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
SExtractor catalog cache: saved Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat to cache
SExtractor catalog cache: saved Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Creating symlink local_wcs_cache/wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits exists and is non-empty
wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits exists and is non-empty
wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits exists and is non-empty
wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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 17:46:40.862 +13:59:59.20
Second-epoch image center 17:46:39.496 +14:01:50.34
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:46:40.862 +13:59:59.20
Second-epoch image center 17:46:37.300 +14:02:03.77
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:46:39.496 +14:01:50.34
Second-epoch second image center 17:46:37.300 +14:02:03.77
Angular distance between the image centers 0.00963 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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits &> /tmp/tmp.mT1ttqdGNb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits &> /tmp/tmp.TtKs34gHRy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits &> /tmp/tmp.F1Y1EvxyN9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits &> /tmp/tmp.iBaU852bbL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits and wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits and wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
Found non-empty wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits and wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
The reference image (wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits) and catalog (wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat) found
'wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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 10341 out of 114670 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.790248
a=0.000000 b=1.000000 c=22.790248
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.09
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.09
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
2.0 pix Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
2.5 pix fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
2.2 pix fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Limiting magnitude estimates:
15.1 mag. Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
15.0 mag. Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
14.5 mag. fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
14.6 mag. fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.9 (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.mT1ttqdGNb (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/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits' -> 'wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WCS_IMAGE_NAME=wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WCS-calibrated image found: wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Checking if the catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits alredy exist and is non-empty...
Catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
WCS catalog name: wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=8242, passed=114655
Got 114655 stars (including 106198 good ones) from the SExtractor catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat
util/solve_plate_with_UCAC5 got 114655 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits -region wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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.TtKs34gHRy (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/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits' -> 'wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WCS_IMAGE_NAME=wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WCS-calibrated image found: wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
Checking if the catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits alredy exist and is non-empty...
Catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat corresponding to the image wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
WCS catalog name: wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=7873, passed=111062
Got 111062 stars (including 103001 good ones) from the SExtractor catalog wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat
util/solve_plate_with_UCAC5 got 111062 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 962 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.38"
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_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits -region wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.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.F1Y1EvxyN9 (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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
WCS_IMAGE_NAME=wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
WCS-calibrated image found: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
Checking if the catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
WCS catalog name: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=4508, passed=71735
Got 71735 stars (including 67149 good ones) from the SExtractor catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat
util/solve_plate_with_UCAC5 got 71735 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits -region wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.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.iBaU852bbL (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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
WCS_IMAGE_NAME=wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
WCS-calibrated image found: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Checking if the catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat corresponding to the image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
WCS catalog name: wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=4875, passed=79151
Got 79151 stars (including 74192 good ones) from the SExtractor catalog wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat
util/solve_plate_with_UCAC5 got 79151 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.60"
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_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits -region wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_Oph-01-Q2b1x1_2026-02-22_06-25-48_20.00sec_-15.00C_LIGHT_0595.fits
Saving fully-calibrated image wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_Oph-01-Q2b1x1_2026-02-22_06-26-26_20.00sec_-15.00C_LIGHT_0596.fits
Saving fully-calibrated image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-20-39_20.00sec_-10.00C_LIGHT_0566.fits
Saving fully-calibrated image wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.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_Oph-01-Q2b1x1_023051_TTUQ2b1x1_5029_ayDSz48U/wcs_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567.fits
Preparing the HTML report for the field Oph-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out131496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131502.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out131532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94600.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131496_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131496_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:07:37.76 +17:31:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 2.150 4502378520929556608 271.90790174504 +17.52297300921 14.0969 13.3686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131497_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131497_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:00:54.82 +16:07:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.175 4501786433917350912 270.22859011134 +16.12447510014 14.2663 13.7272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131499_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131499_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:09:09.78 +13:16:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131502_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131502_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:02:44.38 +10:49:04.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131506_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131506_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:57:44.57 +14:18:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.652 4499828890901906688 269.43538017286 +14.30716410157 13.8589 13.1741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131507_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131507_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:23:11.57 +15:05:39.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131509_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131509_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:53:40.45 +14:07:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.473 4499783875345520384 268.41894750419 +14.12738922940 13.4544 12.9365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131513_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131513_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:10:54.07 +13:36:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.632 4497288331850801024 272.72577200947 +13.61167221351 13.4536 12.6837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131514_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131514_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:58:41.35 +09:55:03.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131517_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131517_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:09:40.57 +14:25:28.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131519_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131519_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:56:32.74 +17:08:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.095 4502737648915543168 269.13673015597 +17.13755329070 13.0558 12.2344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131521_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131521_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:00:44.02 +13:34:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.050 4496718917963832576 270.18360576920 +13.56877351796 13.3825 12.8407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131523_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131523_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:55:30.17 +16:10:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.903 4502514207535525760 268.87617639843 +16.17836077035 13.4388 12.8810 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131527_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131527_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:19:52.10 +11:55:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 0.162 4540517212040146048 259.96706130574 +11.91926607169 13.2062 12.4172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131528_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131528_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:56:37.96 +15:15:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131531_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131531_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:19:11.78 +18:11:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.276 4548257361582544896 259.79901460691 +18.19706794354 12.8896 12.2057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131532_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
Preparing report for the candidate 131532_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131533_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131533_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:11:09.63 +13:51:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131534_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131534_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:56:31.99 +16:56:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 1.208 4502695725733281536 269.13342786372 +16.93357971763 12.5394 12.0503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131535_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131535_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:10:12.53 +16:50:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131537_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131537_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:30:23.45 +17:54:44.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131538_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131538_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:18:18.12 +14:06:07.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131540_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131540_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:09:16.48 +15:14:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131543_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131543_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:11:56.64 +14:46:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.949 4498544038549446144 272.98619556973 +14.77251709257 12.1824 11.3737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131547_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131547_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:07:26.74 +15:21:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.730 4498836749157433344 271.86158113651 +15.36212640212 11.6506 10.9135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131741_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131741_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:02:12.52 +16:29:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131863_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131863_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:59:01.47 +13:52:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.111 4496788736955052800 269.75672477595 +13.88187454263 12.9546 12.3928 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 131915_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131915_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:57:08.51 +13:58:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.224 4499801677988841728 269.28576704425 +13.96942258223 13.2547 12.7985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131917_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131917_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:05:35.93 +17:01:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.819 4502333471011638272 271.39984153115 +17.01990551642 13.2750 12.5595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131937_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131937_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:31:50.26 +11:54:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.360 4493605380210926336 262.95967315630 +11.91341209626 13.0933 12.3542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131973_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131973_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:03:42.13 +12:50:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.822 4496431395673165824 270.92633593451 +12.84578773149 13.2797 12.6885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131991_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131991_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:32:02.58 +16:47:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131993_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131993_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:29:23.47 +11:41:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.253 4493761613940367616 262.34697900314 +11.69096003676 13.7294 13.1725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131997_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 131997_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:03:00.89 +12:37:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.366 4495671156403555968 270.75437606390 +12.62586352101 13.3851 12.5603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132051_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132051_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:01:45.52 +16:38:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.740 4502214762416813568 270.44072672434 +16.64278181556 13.7870 13.3154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132132_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132132_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:59:52.92 +16:35:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132134_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132134_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:55:12.49 +16:14:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132169_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132169_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:53:17.97 +15:18:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132179_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132179_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:59:55.38 +16:30:04.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132217_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132217_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:02:02.09 +17:26:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 2.592 4503080730903234048 270.50933446811 +17.44815349123 14.4069 13.8480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132219_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132219_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:49:13.31 +15:00:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.424 4500838826692332800 267.30551404527 +15.00077139952 14.6743 14.1730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132233_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132233_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:08:34.90 +16:50:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.752 4502085054404164352 272.14537376102 +16.84810069167 14.2242 13.7746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132239_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132239_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:56:21.98 +13:34:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 1.811 4496691297034063360 269.09197612684 +13.57085536385 14.0575 13.2061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132244_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132244_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:47:19.54 +16:13:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 2.950 4501284472498039680 266.83226136317 +16.22820033785 14.2305 13.4581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132247_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132247_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:57:47.93 +14:45:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.625 4499916095918068224 269.44955022469 +14.75077881198 14.4154 13.7560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132248_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132248_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:02:16.77 +18:13:36.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132251_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132251_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:53:15.92 +16:17:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 1.431 4502557363366151424 268.31671298465 +16.28367471306 14.7907 14.4074 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132262_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 132262_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:00:46.80 +15:40:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.741 4501578385701203328 270.19518731172 +15.67453990753 14.5405 13.9247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48379_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 48379_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:00:07.03 +13:02:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80299_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 80299_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:23:18.18 +14:57:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84717_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 84717_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:10:03.50 +18:06:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85277_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 85277_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:48:12.01 +18:04:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46992_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 46992_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:09:20.69 +12:55:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112360_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 112360_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 17:35:40.07 +15:35:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42958_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 42958_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks
**** FOUND 18:07:06.55 +12:33:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94600_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
Preparing report for the candidate 94600_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42058_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567
The candidate 42058_fd_Oph-01-Q2b1x1_2026-03-26_02-24-21_20.00sec_-10.00C_LIGHT_0567 did not pass the final checks