This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz
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
VARIABLE_NAME,2461148.9126,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.4126 11.21CV 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
VARIABLE_NAME,2461148.9126,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.4126 11.49CV 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
VARIABLE_NAME,2461148.9126,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.4126 14.27CV 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
VARIABLE_NAME,2461148.9126,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260418.4126 14.13CV 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: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461148.91294808 18.04.2026 09:54:28.714 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6884
Objects passed selection criteria: 6853
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 4.0 2 4
Average stars detected per image: 5414.5
Average stars matched: 4778.75 (88.2584 %)
Memory usage VmPeak: 114868 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 Sat Apr 18 05:11:18 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: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461148.91294808 18.04.2026 09:54:28.714 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 214
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
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: 20 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): 46131
Objects passed selection criteria: 46004
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 37293
Average stars matched: 32538.5 (87.251 %)
Memory usage VmPeak: 142544 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 Sat Apr 18 05:12:27 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.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: 2461148.91232279
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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits'
wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Image size: 937.4'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 15:07:04.132 -18:01:06.94 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits (1st new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Image size: 937.4'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:34.428 -18:02:22.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:34.428 -18:02:22.42
Angular distance between the image centers 0.1195 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits (2nd new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Image size: 937.4'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:33.454 -18:03:04.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:33.454 -18:03:04.22
Angular distance between the image centers 0.1258 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 15:06:34.428 -18:02:22.42
Second-epoch second image center 15:06:33.454 -18:03:04.22
Angular distance between the image centers 0.01224 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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.a48ih700TJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.GJh4WZJXBV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits &> /tmp/tmp.iEJrD7PREA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits &> /tmp/tmp.v6WkXR1DQx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 6705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 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 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 deg
Loaded 6143 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): 4648 out of 4760 total matches.
Matched with Tycho-2 4760 out of 6705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.861505
a=0.000000 b=1.000000 c=22.861505
From vast_summary.log: estimated ref. image limiting mag.: -8.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.3 pix fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
2.3 pix fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Limiting magnitude estimates:
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.7 mag. fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
14.7 mag. fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.7 (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.a48ih700TJ (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=6705
Got 6705 stars (including 6294 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.GJh4WZJXBV (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=6649
Got 6649 stars (including 6218 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 6649 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.iEJrD7PREA (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=417, passed=7185
Got 7185 stars (including 6761 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 7185 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 7061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 7062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 7062 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.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.v6WkXR1DQx (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=434, passed=7206
Got 7206 stars (including 6768 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 7206 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits'
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21231.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20251_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 20251_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:17:57.84 -13:57:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21007_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
Preparing report for the candidate 21007_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21231_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
Preparing report for the candidate 21231_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21517_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 21517_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:13:35.83 -14:47:10.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:57:43.58 -14:23:10.6
15:10:07.63 -21:05:27.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Image size: 937.4'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 15:07:04.132 -18:01:06.94 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits (1st new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Image size: 937.4'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:34.428 -18:02:22.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:34.428 -18:02:22.42
Angular distance between the image centers 0.1195 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits (2nd new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Image size: 937.4'x624.4' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:33.454 -18:03:04.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:33.454 -18:03:04.22
Angular distance between the image centers 0.1258 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 15:06:34.428 -18:02:22.42
Second-epoch second image center 15:06:33.454 -18:03:04.22
Angular distance between the image centers 0.01224 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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.XsQBnIVAhO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.Bgm57aACej
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits &> /tmp/tmp.NvhTEbi4QZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits &> /tmp/tmp.14mPqSQ7jD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 42407 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 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 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 deg
Loaded 6189 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): 4998 out of 5340 total matches.
Matched with Tycho-2 5340 out of 42407 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.687465
a=0.000000 b=1.000000 c=22.687465
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.72
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 70 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.3 pix fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
2.2 pix fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Limiting magnitude estimates:
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.8 mag. fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
14.8 mag. fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.1 (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.XsQBnIVAhO (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1940, passed=42401
Got 42401 stars (including 40414 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 42401 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.Bgm57aACej (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1927, passed=42823
Got 42823 stars (including 40848 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 42823 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.NvhTEbi4QZ (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=2450, passed=46025
Got 46025 stars (including 43512 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 46025 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 45488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 45493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 45494 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.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.14mPqSQ7jD (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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=2323, passed=46243
Got 46243 stars (including 43852 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 46243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 45728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 45727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 45727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-53-34_20.00sec_-5.00C_LIGHT_0221.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.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_2026-04-18_CI_Lib-03-Q2b1x1_050423_TTUQ2b1x1_2152300_bea1rDiz/wcs_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222.fits
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out61647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61740.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: 1s
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Considering the candidate 53036_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53036_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:05:54.34 -22:15:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.825 6231425766090009984 226.47660648244 -22.25379723428 14.1458 13.6007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53037_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53037_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:17:02.61 -20:44:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.424 6253060375353450880 229.26018668529 -20.74330864345 13.9754 13.3803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53038_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53038_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:07:21.60 -18:33:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53039_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53039_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:06.04 -14:06:01.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53041_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53041_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:15:21.04 -14:05:49.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53045_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53045_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:21:59.16 -18:49:02.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53047_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53047_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:16:40.99 -19:00:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53057_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53057_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:14.03 -22:09:14.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53060_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53060_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:22:48.42 -20:09:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53063_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53063_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:23:19.99 -20:28:09.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53825_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 53825_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 14:57:43.58 -14:23:10.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54023_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 54023_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:10:07.62 -21:05:27.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55466_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 55466_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 14:50:34.83 -16:00:52.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56827_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 56827_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:17:24.90 -17:13:56.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58171_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 58171_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:22:53.49 -22:05:02.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58180_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 58180_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:20:36.06 -19:39:28.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58506_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 58506_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:18.86 -21:26:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58869_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 58869_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:54.94 -22:01:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59156_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59156_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:23:13.03 -21:40:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59214_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59214_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:20:23.99 -15:41:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59436_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59436_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:46.16 -21:25:15.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59496_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59496_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:49.91 -22:04:49.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59568_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59568_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:18:09.88 -21:52:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59664_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59664_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:21:57.22 -21:49:18.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59812_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59812_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:20:51.61 -21:45:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59952_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 59952_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:14.20 -22:02:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60087_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60087_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:18:05.67 -21:39:55.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60281_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60281_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:25.70 -18:11:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.118 6257951179173417728 231.35740074154 -18.18707368744 13.9349 13.2777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60408_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60408_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:21.41 -21:49:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60535_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60535_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:05:26.83 -20:47:38.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60678_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60678_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:23:20.88 -22:09:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.460 6251917093719536896 230.83702271834 -22.15667962886 13.8429 13.2294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60766_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60766_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:41.53 -19:52:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60851_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60851_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:57.29 -22:09:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.554 6251873250693627776 231.23837357977 -22.15760583537 13.9195 13.2219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60881_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60881_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:46.07 -21:39:17.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60887_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60887_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:18:22.53 -18:04:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.503 6258131808313752192 229.59374060359 -18.07813756503 14.4799 14.0182 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60986_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 60986_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:57.70 -21:02:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.454 6252847417996505472 231.24000861052 -21.03580985242 13.8566 13.3164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61014_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61014_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:22:33.79 -15:49:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61103_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61103_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 14:57:03.14 -16:18:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61128_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61128_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:35.92 -22:02:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61190_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61190_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:20:04.53 -22:03:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.376 6252320305252555136 230.01847976078 -22.06463735637 14.1136 13.5731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61247_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61247_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:40.00 -21:26:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.139 6252073808486090112 231.41665728082 -21.44510115537 13.9810 13.3305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.139#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61272_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61272_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:22:06.83 -21:36:26.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61410_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61410_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:20:10.09 -21:12:25.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61423_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61423_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:31.79 -21:55:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.562 6251928187615061120 231.13231014266 -21.92326862949 14.3592 13.4182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61469_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61469_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:22:58.17 -21:38:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61492_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61492_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:13.23 -14:10:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.604 6266040488076772224 231.30518152465 -14.17906355331 14.2794 13.7016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61574_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61574_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:19:22.98 -22:13:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61578_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61578_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:16:50.24 -20:49:57.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61634_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61634_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:17:21.14 -22:10:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.697 6252257358211963136 229.33788141490 -22.17305036380 14.0584 13.3558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61647_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
Preparing report for the candidate 61647_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61672_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61672_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:20:47.30 -22:04:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61685_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61685_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:01:53.63 -14:47:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61691_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61691_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:09.09 -22:01:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61740_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
Preparing report for the candidate 61740_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
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Considering the candidate 61768_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61768_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:18:55.47 -16:54:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.430 6259104463787335040 229.73107909581 -16.91083330742 14.1812 13.6188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61788_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61788_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:25:41.29 -15:32:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.682 6259690709643625600 231.42185218072 -15.53497736785 14.4424 13.9170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61793_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61793_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:24:17.72 -21:45:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.575 6251968289730126464 231.07367750921 -21.75548790966 13.9587 13.2218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 61847_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61847_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:20:28.81 -21:42:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61901_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61901_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:22:23.77 -20:56:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61906_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61906_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:18:53.31 -17:33:23.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)
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Considering the candidate 61998_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 61998_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:15:04.46 -20:23:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62003_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 62003_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:06:07.63 -21:19:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62024_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 62024_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:12:49.63 -20:02:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.729 6255984324665615744 228.20655342913 -20.04421092620 14.4302 13.7670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62058_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 62058_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:19:18.26 -22:06:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62104_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 62104_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:09:08.56 -22:11:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62252_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 62252_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 15:09:27.14 -21:38:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.33, MAG_FAINT_SEARCH_LIMIT=15.31)GAIADR2_OUTPUT=# 0.873 6231552454742224896 227.36321795089 -21.63565343646 14.2319 13.7226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 62581_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 62581_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 14:49:26.67 -21:34:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62626_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 62626_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 14:59:51.41 -21:37:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.155 6232446529493868416 224.96394367101 -21.63006695065 14.1231 13.3719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 63027_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 63027_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks
**** FOUND 14:50:04.93 -21:41:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23565_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222
The candidate 23565_fd_Lib-03-Q2b1x1_2026-04-18_04-54-28_20.00sec_-4.90C_LIGHT_0222 did not pass the final checks