This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 10.1181 2461231.6181 12.01 15:05:22.29 -36:15:32.4
331.03516 19.19972 galactic Lup Second-epoch detections are separated by 1.1" and 8.0 pix
The object was found in VSX 1" V0346 Lup
Type: LB
# Max. Min./Amp. JD0 Period
12.000 V 14.100 V 2452268.10000 164.051819000000
The object was not found in astcheck.
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 15:05:22.29 -36:15:32.4: 13.23 +/- 0.12 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 15:05:22.29 -36:15:32.4: 13.48 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.10
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0346 Lup,2461231.6181,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0346 Lup 20260710.1181 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 10.1181 2461231.6181 11.63 15:05:12.91 -36:18:05.8
330.98322 19.17969 galactic Lup Second-epoch detections are separated by 2.6" and 8.2 pix
The object was found in VSX 3" ASASSN-V J150512.72-361804.6
Type: L
# Max. Min./Amp. JD0 Period
12.950 V 13.520 V
The object was not found in astcheck.
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 15:05:12.91 -36:18:05.8: 12.50 +/- 0.06 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 15:05:12.91 -36:18:05.8: 12.57 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.05
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin Lite
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J150512.72-361804.6,2461231.6181,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J150512.72-361804.6 20260710.1181 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461180.75420722 20.05.2026 06:05:53.504 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
First image: 2461180.75420722 20.05.2026 06:05:53.504 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Last image: 2461231.61841793 10.07.2026 02:50:21.309 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.43
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: 3 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): 5015
Objects passed selection criteria: 4998
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 3641
Average stars matched: 3540.75 (97.2466 %)
Memory usage VmPeak: 111352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 9 21:52:14 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: 2461180.75420722 20.05.2026 06:05:53.504 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
First image: 2461180.75420722 20.05.2026 06:05:53.504 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Last image: 2461231.61841793 10.07.2026 02:50:21.309 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.08
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: 17 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): 52219
Objects passed selection criteria: 52125
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 38234.2
Average stars matched: 36550.8 (95.5969 %)
Memory usage VmPeak: 154616 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 8 15:05:08 CDT 2026
VaST build number 1.0rc89-141-gc31ee76a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 9 21:54:24 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.cat to cache
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.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/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.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: 2461231.61772194
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits exists and is non-empty
Saving wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits to local_wcs_cache/
'wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits' -> 'local_wcs_cache/wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits'
wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits exists and is non-empty
Saving wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits to local_wcs_cache/
'wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits' -> 'local_wcs_cache/wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits'
wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits exists and is non-empty
Saving wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits to local_wcs_cache/
'wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits' -> 'local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits'
wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits exists and is non-empty
Saving wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits to local_wcs_cache/
'wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits' -> 'local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits (1st reference image)
verification OK: wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Image size: 937.3'x625.1' 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: 15:39:09.271 -34:00:32.00 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_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits (1st new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Image size: 940.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:39:08.448 -34:00:04.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:39:09.271 -34:00:32.00
Second-epoch image center 15:39:08.448 -34:00:04.57
Angular distance between the image centers 0.0081 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits (2nd new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Image size: 940.6'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:39:10.227 -33:59:26.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:39:09.271 -34:00:32.00
Second-epoch image center 15:39:10.227 -33:59:26.19
Angular distance between the image centers 0.0186 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 15:39:08.448 -34:00:04.57
Second-epoch second image center 15:39:10.227 -33:59:26.19
Angular distance between the image centers 0.01231 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits &> /tmp/tmp.rnFGzp3WnI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits &> /tmp/tmp.JbflfOqBKv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits &> /tmp/tmp.UdSYBRGf9K
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits &> /tmp/tmp.eMfMwqzljD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.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_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits and wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits and wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
Found non-empty wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits and wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
The reference image (wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits) and catalog (wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat) found
'wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat' -> 'wcsmag.cat'
Read 5307 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.8428 to 244.7912 deg, Dec -39.2751 to -28.4897 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 224.8428 to 244.7912 deg, Dec -39.2751 to -28.4897 deg
Loaded 10291 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): 4394 out of 4486 total matches.
Matched with Tycho-2 4486 out of 5307 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.318400
a=0.000000 b=1.000000 c=22.318400
From vast_summary.log: estimated ref. image limiting mag.: -8.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.89
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5307 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.8428 to 244.7912 deg, Dec -39.2751 to -28.4897 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 224.8428 to 244.7912 deg, Dec -39.2751 to -28.4897 deg
Loaded 10291 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): 4394 out of 4486 total matches.
Matched with Tycho-2 4486 out of 5307 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits (aperture=6.2)
Read 5327 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.8427 to 244.7921 deg, Dec -39.2750 to -28.4897 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 224.8427 to 244.7921 deg, Dec -39.2750 to -28.4897 deg
Loaded 10291 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): 4420 out of 4513 total matches.
Matched with Tycho-2 4513 out of 5327 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
2.2 pix Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
3.0 pix fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
2.9 pix fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
2.2 pix wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
2.2 pix wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
Limiting magnitude estimates:
13.9 mag. Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
13.9 mag. Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
12.7 mag. fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
12.8 mag. fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 10.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rnFGzp3WnI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits' -> 'wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=372, bad_region=0, passed=5307
Got 5307 stars (including 4930 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
util/solve_plate_with_UCAC5 got 5307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits N_match=961 sigma_overall_arcsec=0.596 sigma_q1_arcsec=0.507 sigma_q2_arcsec=0.896 sigma_q3_arcsec=0.662 sigma_q4_arcsec=0.609 n_q1=251 n_q2=228 n_q3=194 n_q4=288 worst_quadrant_to_overall_ratio=1.504
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits -region wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JbflfOqBKv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits' -> 'wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=375, bad_region=0, passed=5327
Got 5327 stars (including 4944 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat
util/solve_plate_with_UCAC5 got 5327 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 960 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(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 5227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 960 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(), 5227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 5227 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits N_match=958 sigma_overall_arcsec=0.613 sigma_q1_arcsec=0.508 sigma_q2_arcsec=0.799 sigma_q3_arcsec=0.687 sigma_q4_arcsec=0.611 n_q1=247 n_q2=224 n_q3=202 n_q4=285 worst_quadrant_to_overall_ratio=1.302
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits -region wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UdSYBRGf9K (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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=296, bad_region=0, passed=1955
Got 1955 stars (including 1657 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 1955 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010452 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.0)
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: 957 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 1919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.0)
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: 957 matched stars entering correct_measured_positions(), 1917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 1917 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! :)
WCS_QUALITY_DIAG: file=fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits N_match=957 sigma_overall_arcsec=0.479 sigma_q1_arcsec=0.565 sigma_q2_arcsec=0.630 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.416 n_q1=234 n_q2=207 n_q3=234 n_q4=282 worst_quadrant_to_overall_ratio=1.317
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eMfMwqzljD (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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=270, bad_region=0, passed=2072
Got 2072 stars (including 1802 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 2072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.6'
Seting catalog search parameters based on the expected field of view 940.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013064 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010451 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.0)
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: 957 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 2042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.0)
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: 957 matched stars entering correct_measured_positions(), 2042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 2042 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits N_match=957 sigma_overall_arcsec=0.484 sigma_q1_arcsec=0.605 sigma_q2_arcsec=0.564 sigma_q3_arcsec=0.435 sigma_q4_arcsec=0.385 n_q1=236 n_q2=208 n_q3=224 n_q4=289 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits sigma_overall=0.596 worst_q_ratio=1.504
ref2=Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits sigma_overall=0.613 worst_q_ratio=1.302
new1=fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits sigma_overall=0.479 worst_q_ratio=1.317
new2=fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits sigma_overall=0.484 worst_q_ratio=1.250
reference average sigma_overall=0.6045 worst_q_ratio=1.403
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230_astrometric_residuals.png (961 matched stars from wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231_astrometric_residuals.png (958 matched stars from wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000_astrometric_residuals.png (957 matched stars from wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001_astrometric_residuals.png (957 matched stars from wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.45 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits'
Saving fully-calibrated image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits'
Preparing the HTML report for the field Lup-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20362_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 20362_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:25:47.60 -36:13:53.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01642_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 01642_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:53:28.87 -36:17:52.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Lup-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.cat to cache
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Creating symlink local_wcs_cache/wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
Creating symlink local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Creating symlink local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.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_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits exists and is non-empty
wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits exists and is non-empty
wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits exists and is non-empty
wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits (1st reference image)
verification OK: wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Image size: 937.3'x625.1' 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: 15:39:09.271 -34:00:32.00 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_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits (1st new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Image size: 940.7'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:39:08.448 -34:00:04.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:39:09.271 -34:00:32.00
Second-epoch image center 15:39:08.448 -34:00:04.57
Angular distance between the image centers 0.0081 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits (2nd new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Image size: 940.6'x627.2' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:39:10.227 -33:59:26.19 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:39:09.271 -34:00:32.00
Second-epoch image center 15:39:10.227 -33:59:26.19
Angular distance between the image centers 0.0186 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 15:39:08.448 -34:00:04.57
Second-epoch second image center 15:39:10.227 -33:59:26.19
Angular distance between the image centers 0.01231 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits &> /tmp/tmp.oOP0fKooWt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits &> /tmp/tmp.K7NZIzXY3d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits &> /tmp/tmp.2TAnM1qCh9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits &> /tmp/tmp.6LqFBh0GdA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.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_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits and wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits and wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
Found non-empty wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits and wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
The reference image (wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits) and catalog (wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat) found
'wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat' -> 'wcsmag.cat'
Read 57659 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.7646 to 244.7912 deg, Dec -39.2842 to -28.4668 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 224.7646 to 244.7912 deg, Dec -39.2842 to -28.4668 deg
Loaded 10349 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): 8059 out of 8697 total matches.
Matched with Tycho-2 8697 out of 57659 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.114000
a=0.000000 b=1.000000 c=22.114000
From vast_summary.log: estimated ref. image limiting mag.: -8.08
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.03
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 57659 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.7646 to 244.7912 deg, Dec -39.2842 to -28.4668 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 224.7646 to 244.7912 deg, Dec -39.2842 to -28.4668 deg
Loaded 10349 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): 8059 out of 8697 total matches.
Matched with Tycho-2 8697 out of 57659 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits (aperture=4.5)
Read 58252 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.7644 to 244.7921 deg, Dec -39.2885 to -28.4858 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 224.7644 to 244.7921 deg, Dec -39.2885 to -28.4858 deg
Loaded 10341 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): 8042 out of 8697 total matches.
Matched with Tycho-2 8697 out of 58252 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
2.0 pix Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
2.6 pix fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
2.6 pix fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
2.0 pix wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
2.0 pix wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
Limiting magnitude estimates:
14.0 mag. Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
14.0 mag. Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
12.9 mag. fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
12.9 mag. fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oOP0fKooWt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits' -> 'wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2382, bad_region=3, passed=57646
Got 57646 stars (including 55161 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat
util/solve_plate_with_UCAC5 got 57646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 960 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(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 56559 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 960 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(), 56561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 56562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits N_match=957 sigma_overall_arcsec=0.582 sigma_q1_arcsec=0.508 sigma_q2_arcsec=0.813 sigma_q3_arcsec=0.623 sigma_q4_arcsec=0.589 n_q1=252 n_q2=225 n_q3=188 n_q4=292 worst_quadrant_to_overall_ratio=1.397
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits -region wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.K7NZIzXY3d (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits' -> 'wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=4, blended=2461, bad_region=1, passed=58247
Got 58247 stars (including 55716 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat
util/solve_plate_with_UCAC5 got 58247 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 253 to 309 (Dec -39.3 to -28.5)
Done reading UCAC5 zone files...
Matched 960 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(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 57286 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 253 to 309 (Dec -39.3 to -28.5)
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: 957 matched stars entering correct_measured_positions(), 57288 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 57289 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits N_match=957 sigma_overall_arcsec=0.592 sigma_q1_arcsec=0.480 sigma_q2_arcsec=0.773 sigma_q3_arcsec=0.640 sigma_q4_arcsec=0.611 n_q1=248 n_q2=225 n_q3=186 n_q4=298 worst_quadrant_to_overall_ratio=1.305
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits -region wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2TAnM1qCh9 (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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=592, bad_region=1, passed=18532
Got 18532 stars (including 17917 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 18532 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010452 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.0)
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: 954 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 18255 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 252 to 311 (Dec -39.4 to -28.0)
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: 954 matched stars entering correct_measured_positions(), 18257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 18257 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits N_match=954 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.564 sigma_q2_arcsec=0.593 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.412 n_q1=207 n_q2=197 n_q3=241 n_q4=309 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6LqFBh0GdA (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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=572, bad_region=1, passed=19632
Got 19632 stars (including 19028 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 19632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.6'
Seting catalog search parameters based on the expected field of view 940.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013064 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010451 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 312 (Dec -39.4 to -28.0)
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: 954 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 19354 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 252 to 311 (Dec -39.4 to -28.0)
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: 954 matched stars entering correct_measured_positions(), 19356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 19356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits N_match=954 sigma_overall_arcsec=0.472 sigma_q1_arcsec=0.564 sigma_q2_arcsec=0.583 sigma_q3_arcsec=0.458 sigma_q4_arcsec=0.396 n_q1=213 n_q2=195 n_q3=239 n_q4=307 worst_quadrant_to_overall_ratio=1.234
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-49-21_20.00sec_-0.00C_LIGHTs_0000.fits
Saving fully-calibrated image wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.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_2026-07-09_CI_Lup-01-Q1b1x1_215104_TTUQ1b1x1_166777_ETuXpUbI/wcs_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001.fits
Preparing the HTML report for the field Lup-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 15:36:45.51 -28:51:34.2: 11.44 +/- 0.02 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 16:09:14.07 -32:06:34.6: 12.25 +/- 0.05 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 15:00:39.94 -36:38:13.2: 11.25 +/- 0.02 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 15:48:26.84 -32:04:47.8: 12.46 +/- 0.05 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 15:36:45.51 -28:51:34.2: 11.44 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.44 +/- 0.01
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 16:09:14.07 -32:06:34.6: 12.26 +/- 0.05 detection
Forced photometry filter REJECTED candidate at 15:36:45.51 -28:51:34.2: ref_mag=11.44 +/- 0.01 new_mean_mag=11.4972 delta=-0.06 (need > 0.90)
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 15:05:22.29 -36:15:32.4: 13.23 +/- 0.12 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 15:00:39.94 -36:38:13.2: 11.27 +/- 0.02 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-05-53_20.00sec_4.90C_LIGHT_0230.fits at 15:05:12.91 -36:18:05.8: 12.50 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.26 +/- 0.04
Forced photometry filter REJECTED candidate at 16:09:14.07 -32:06:34.6: ref_mag=12.26 +/- 0.04 new_mean_mag=12.1798 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 11.26 +/- 0.02
Forced photometry filter REJECTED candidate at 15:00:39.94 -36:38:13.2: ref_mag=11.26 +/- 0.02 new_mean_mag=11.4685 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 15:48:26.84 -32:04:47.8: 12.59 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.52 +/- 0.04
Forced photometry filter REJECTED candidate at 15:48:26.84 -32:04:47.8: ref_mag=12.52 +/- 0.04 new_mean_mag=12.6203 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 15:05:22.29 -36:15:32.4: 13.48 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.32 +/- 0.10
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-20_01-06-47_20.00sec_4.90C_LIGHT_0231.fits at 15:05:12.91 -36:18:05.8: 12.57 +/- 0.07 detection
Forced photometry filter KEPT candidate at 15:05:22.29 -36:15:32.4: ref_mag=13.32 +/- 0.10 new_mean_mag=12.0067 delta=1.32 (need > 0.90)
Forced photometry reference-image weighted average: 12.53 +/- 0.05
Forced photometry filter KEPT candidate at 15:05:12.91 -36:18:05.8: ref_mag=12.53 +/- 0.05 new_mean_mag=11.6329 delta=0.90 (need > 0.90)
Adding exclusion_list_local.txt__out13888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14200.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 73744_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 73744_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 73793_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 73793_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:07:04.78 -28:31:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73889_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 73889_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 73934_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 73934_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:49:33.20 -31:04:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73962_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 73962_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:51:06.87 -31:35:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74027_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 74027_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:24:02.32 -36:59:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74029_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 74029_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:30:44.37 -38:20:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74040_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 74040_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:02:58.46 -35:51:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74115_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 74115_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 74229_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 74229_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:01:23.51 -31:51:51.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74277_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 74277_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 01334_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 01334_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:16:00.12 -38:38:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13732_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 13732_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:53:08.20 -36:34:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20753_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 20753_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:40:11.43 -35:15:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14200_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 14200_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 13888_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
Preparing report for the candidate 13888_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
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Considering the candidate 67915_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 67915_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:25:47.61 -36:13:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02743_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 02743_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:33:17.04 -38:42:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48443_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 48443_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:56:47.09 -30:41:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41818_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 41818_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:51:24.14 -32:51:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15127_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 15127_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:53:28.88 -36:17:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35847_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 35847_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:55:38.24 -29:15:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05830_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 05830_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:26:26.60 -38:06:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18388_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 18388_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:38:51.08 -35:44:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06608_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001
The candidate 06608_fd_Lup-01-Q1b1x1_2026-07-09_21-50-21_20.00sec_0.00C_LIGHTs_0001 did not pass the final checks