This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J191122.10+130628.7,2461150.9673,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
ZTF J191122.10+130628.7 20260420.4673 12.45CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 11296553,2461150.9673,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 11296553 20260420.4673 12.54CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
First image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Last image: 2461150.96763392 20.04.2026 11:13:13.571 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.05
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: 6 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): 20769
Objects passed selection criteria: 20688
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 14355
Average stars matched: 13830 (96.3427 %)
Memory usage VmPeak: 125268 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 07:02:35 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: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
First image: 2461098.99746946 27.02.2026 11:56:11.361 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Last image: 2461150.96763392 20.04.2026 11:13:13.571 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 72
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 82 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): 211928
Objects passed selection criteria: 211421
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 152060
Average stars matched: 145224 (95.5044 %)
Memory usage VmPeak: 2033188 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 20 07:09:01 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
SExtractor catalog cache: saved Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.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: 2461150.96689569
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'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
Saving wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits to local_wcs_cache/
'wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> 'local_wcs_cache/wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits'
wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits exists and is non-empty
Saving wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits to local_wcs_cache/
'wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits' -> 'local_wcs_cache/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits (1st reference image)
verification OK: wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Image size: 942.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:21.178 +14:00:13.40 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits (1st new image)
verification OK: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:27.040 +13:59:19.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:27.040 +13:59:19.34
Angular distance between the image centers 0.0281 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits (2nd new image)
verification OK: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:29.563 +13:58:37.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:29.563 +13:58:37.27
Angular distance between the image centers 0.0432 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 19:33:27.040 +13:59:19.34
Second-epoch second image center 19:33:29.563 +13:58:37.27
Angular distance between the image centers 0.01551 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/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.fgEQE7MBA7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.1g2FzHOfF5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits &> /tmp/tmp.xK5vOBpytB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits &> /tmp/tmp.o7GgLh2yi6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
Found non-empty wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
The reference image (wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits) and catalog (wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat) found
'wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat' -> 'wcsmag.cat'
Read 22299 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.9644 to 301.5045 deg, Dec +8.4825 to +19.3280 deg
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
Tycho-2 catalog search boundaries: RA 284.9644 to 301.5045 deg, Dec 8.4825 to 19.3280 deg
Loaded 19314 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 10832 out of 11734 total matches.
Matched with Tycho-2 11734 out of 22299 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.853200
a=0.000000 b=1.000000 c=22.853200
From vast_summary.log: estimated ref. image limiting mag.: -8.05
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
2.2 pix Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
2.5 pix fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
2.4 pix fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Limiting magnitude estimates:
14.8 mag. Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
14.8 mag. Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
13.9 mag. fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
14.0 mag. fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.1 (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.fgEQE7MBA7 (6) ############
Parsing command line arguments...
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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> 'wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2194, passed=22299
Got 22299 stars (including 20069 good ones) from the SExtractor catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 22299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 21165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 21166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 21166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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.1g2FzHOfF5 (6) ############
Parsing command line arguments...
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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2174, passed=22325
Got 22325 stars (including 20124 good ones) from the SExtractor catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 22325 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 21080 with non-zero local correction accuracy
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...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 21084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 966 matched stars entering correct_measured_positions(), 21084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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.xK5vOBpytB (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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Checking if the catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
WCS catalog name: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=349, passed=5840
Got 5840 stars (including 5484 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat
util/solve_plate_with_UCAC5 got 5840 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.4)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.4)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5453 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits -region wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.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.o7GgLh2yi6 (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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Checking if the catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
WCS catalog name: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=459, passed=7302
Got 7302 stars (including 6835 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat
util/solve_plate_with_UCAC5 got 7302 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6878 with non-zero local correction accuracy
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...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.6)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 6875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits -region wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.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_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
Saving fully-calibrated image wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits'
Saving fully-calibrated image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits'
Preparing the HTML report for the field Aql-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31860.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 31809_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31809_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:33:42.88 +13:01:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31814_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31814_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:33:05.09 +12:45:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31824_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31824_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:32:16.79 +11:47:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31829_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31829_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:31:36.21 +12:23:21.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31831_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31831_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:31:22.04 +12:23:34.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31834_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31834_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:31:24.37 +12:39:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31842_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31842_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:34:10.41 +12:56:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.349 4316289751394526720 293.54312454448 +12.93603428126 11.9758 11.7515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31846_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31846_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:32:58.12 +11:58:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31853_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31853_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:32:57.33 +12:08:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.373 4315401723933588992 293.23873796325 +12.14882935941 11.1610 9.9999 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31860_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 31860_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:31:48.97 +12:19:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 0.928 4315421309029935104 292.95400980046 +12.32425602982 11.3500 10.3260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.928#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 Aql-01-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
SExtractor catalog cache: saved Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat to cache
SExtractor catalog cache: saved Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Creating symlink local_wcs_cache/wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.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_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits exists and is non-empty
wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits (1st reference image)
verification OK: wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Image size: 942.0'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:21.178 +14:00:13.40 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits (1st new image)
verification OK: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:27.040 +13:59:19.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:27.040 +13:59:19.34
Angular distance between the image centers 0.0281 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits (2nd new image)
verification OK: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Image size: 941.1'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:33:29.563 +13:58:37.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:21.178 +14:00:13.40
Second-epoch image center 19:33:29.563 +13:58:37.27
Angular distance between the image centers 0.0432 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 19:33:27.040 +13:59:19.34
Second-epoch second image center 19:33:29.563 +13:58:37.27
Angular distance between the image centers 0.01551 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/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.WPDqYkzetu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.L4SC9pwpN5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits &> /tmp/tmp.FnQ3oQAY8w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits &> /tmp/tmp.X7GijAgZhZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
Found non-empty wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits and wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
The reference image (wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits) and catalog (wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat) found
'wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat' -> 'wcsmag.cat'
Read 233554 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.9240 to 301.5198 deg, Dec +8.4825 to +19.3288 deg
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
Tycho-2 catalog search boundaries: RA 284.9240 to 301.5198 deg, Dec 8.4825 to 19.3288 deg
Loaded 19362 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9628 out of 13769 total matches.
Matched with Tycho-2 13769 out of 233554 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.676529
a=0.000000 b=1.000000 c=22.676529
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.96
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.96
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
2.0 pix Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
2.3 pix fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
2.2 pix fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Limiting magnitude estimates:
15.0 mag. Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
15.0 mag. Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
14.2 mag. fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
14.2 mag. fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.4 (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.WPDqYkzetu (6) ############
Parsing command line arguments...
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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits' -> 'wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=33990, passed=233496
Got 233496 stars (including 199148 good ones) from the SExtractor catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 233496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 225537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 225536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 225537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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.L4SC9pwpN5 (6) ############
Parsing command line arguments...
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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits' -> 'wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=75, blended=33841, passed=234240
Got 234240 stars (including 200019 good ones) from the SExtractor catalog wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 234240 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 226322 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 226324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 226231 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 973 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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.FnQ3oQAY8w (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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Checking if the catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
WCS catalog name: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=3, blended=4977, passed=64261
Got 64261 stars (including 59206 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat
util/solve_plate_with_UCAC5 got 64261 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 60295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 60298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 60298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits -region wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.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.X7GijAgZhZ (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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
WCS_IMAGE_NAME=wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
WCS-calibrated image found: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Checking if the catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat corresponding to the image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
WCS catalog name: wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=6361, passed=79455
Got 79455 stars (including 72985 good ones) from the SExtractor catalog wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat
util/solve_plate_with_UCAC5 got 79455 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 74403 with non-zero local correction accuracy
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...
Searching UCAC5 zones 490 to 550 (Dec 8.1 to 19.6)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 74404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 74404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits -region wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.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_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_Aql-01-Q1b1x1_2026-02-27_05-56-11_20.00sec_-15.00C_LIGHT_0047.fits
Saving fully-calibrated image wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_Aql-01-Q1b1x1_2026-02-27_05-57-08_20.00sec_-14.90C_LIGHT_0048.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-12-09_20.00sec_-4.90C_LIGHTs_0050.fits
Saving fully-calibrated image wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.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_2026-04-20_CI_Aql-01-Q1b1x1_061413_TTUQ1b1x1_510059_fzZlMFgC/wcs_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051.fits
Preparing the HTML report for the field Aql-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out267639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out267810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out268663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out267910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90342.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
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Considering the candidate 267639_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267639_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:43:40.92 +17:46:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.321 1824104947475204736 295.92091588598 +17.78084202115 13.7526 12.8222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267658_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267658_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:41:46.71 +17:51:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.368 1824077150462352384 295.44457541040 +17.85847951007 13.4631 12.5914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267666_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267666_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:41:25.93 +15:56:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267676_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267676_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:07:12.35 +11:26:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.642 4312702079311028224 286.80186047943 +11.45009089416 12.9399 11.7132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 267688_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267688_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:34:49.98 +13:30:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267693_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267693_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:07:00.61 +13:59:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.605 4314418760580856576 286.75270292111 +13.98611716242 11.7572 10.5290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267697_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267697_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:09:14.90 +12:59:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267704_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267704_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:39:06.47 +15:38:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.104 4318724997851243392 294.77664256381 +15.64501583814 12.0859 11.3110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267708_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267708_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:50:47.89 +08:52:17.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 267810_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267810_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:39:45.76 +16:47:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 0.771 4321944844582689792 294.94088502434 +16.78399092886 11.5589 10.5918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 267854_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267854_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:47:30.19 +18:29:56.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 267881_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 267881_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:32:03.20 +11:43:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 267910_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
Preparing report for the candidate 267910_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
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Considering the candidate 268068_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268068_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:09:38.81 +11:06:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268070_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268070_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:38:29.72 +17:14:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268092_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268092_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:37:50.98 +12:47:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268098_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268098_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:47:32.55 +18:29:39.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 268152_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268152_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:34:49.89 +13:03:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268156_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268156_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:39:22.83 +17:08:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268163_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268163_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:39:01.64 +16:54:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268164_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268164_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:08:24.81 +13:04:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268178_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268178_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:29:50.99 +09:59:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268202_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268202_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:31:51.14 +11:19:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268210_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268210_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:24:30.67 +12:15:44.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 268213_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268213_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:39:26.58 +17:08:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268291_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268291_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:31:16.33 +10:12:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268321_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268321_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:34:50.99 +12:03:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268371_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268371_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:43:28.37 +18:17:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268375_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268375_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:29:39.25 +12:23:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268381_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268381_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:24:25.68 +11:01:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268388_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268388_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:47:27.09 +18:29:43.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 268396_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268396_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:34:06.45 +12:33:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268419_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268419_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:32:50.29 +12:50:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268434_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268434_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:20:33.47 +09:45:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268438_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268438_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:47:30.64 +18:20:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268451_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268451_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:33:41.52 +12:57:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268467_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268467_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:01:26.88 +11:28:37.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 268484_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268484_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:08:03.45 +11:27:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268589_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268589_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:37:47.34 +12:55:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 268641_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268641_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:20:30.90 +13:06:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.332 4319167035843083904 290.12891631533 +13.11521693143 12.3481 11.0480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 268663_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268663_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:39:44.79 +15:56:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.640 4318739978697970176 294.93639391602 +15.94203653574 13.9496 13.0430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 268813_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 268813_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:30:17.31 +11:25:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 256267_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 256267_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:31:04.32 +12:09:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90342_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
Preparing report for the candidate 90342_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
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Considering the candidate 20126_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 20126_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:22:03.11 +09:42:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59392_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 59392_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:27:20.27 +11:39:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244172_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 244172_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:29:55.95 +11:36:23.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 218690_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 218690_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:05:00.98 +18:02:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65772_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 65772_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks
**** FOUND 19:32:22.98 +11:59:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232202_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051
The candidate 232202_fd_Aql-01-Q1b1x1_2026-04-20_06-13-13_20.00sec_-4.90C_LIGHTs_0051 did not pass the final checks