This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B
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 07.1186 2461228.6186 11.05 15:18:02.49 -37:50:20.5
332.38397 16.50938 galactic Lup Second-epoch detections are separated by 0.7" and 6.0 pix
The object was found in VSX 2" ASAS J151802-3750.4
Type: MISC
# Max. Min./Amp. JD0 Period
8.689 Ic Y 0.393 Ic 2455121.20000 1078.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits at 15:18:02.49 -37:50:20.5: 11.97 +/- 0.03 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits at 15:18:02.49 -37:50:20.5: 12.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.03
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
ASAS J151802-3750.4,2461228.6186,11.05,0.05,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
ASAS J151802-3750.4 20260707.1186 11.05CV 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 07.1186 2461228.6186 11.78 15:44:35.48 -37:59:29.0
336.65982 13.29011 galactic Lup Second-epoch detections are separated by 2.1" and 6.2 pix
The object was found in VSX 1" ASASSN-V J154435.52-375928.2
Type: L
# Max. Min./Amp. JD0 Period
13.150 V 13.620 V
The object was not found in astcheck.
Forced photometry on wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits at 15:44:35.48 -37:59:29.0: 12.86 +/- 0.06 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits at 15:44:35.48 -37:59:29.0: 12.97 +/- 0.10 detection
Forced photometry reference-image weighted average: 12.89 +/- 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 J154435.52-375928.2,2461228.6186,11.78,0.05,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 J154435.52-375928.2 20260707.1186 11.78CV 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: 2461146.81684877 16.04.2026 07:36:05.734 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
First image: 2461146.81684877 16.04.2026 07:36:05.734 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Last image: 2461228.61889862 07.07.2026 02:51:02.841 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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.: -8.48
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): 5045
Objects passed selection criteria: 5037
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: 4028
Average stars matched: 3975 (98.6842 %)
Memory usage VmPeak: 112176 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jul 6 21:07:40 CDT 2026
VaST build number 1.0rc89-130-g0d8e31cd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 6 21:53:07 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: 2461146.81684877 16.04.2026 07:36:05.734 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
First image: 2461146.81684877 16.04.2026 07:36:05.734 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Last image: 2461228.61889862 07.07.2026 02:51:02.841 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.13
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: 13 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): 45374
Objects passed selection criteria: 45312
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 36599.8
Average stars matched: 36042 (98.4761 %)
Memory usage VmPeak: 156692 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jul 6 21:07:40 CDT 2026
VaST build number 1.0rc89-130-g0d8e31cd
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jul 6 21:55:18 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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.cat to cache
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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: 2461228.61836458
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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits exists and is non-empty
Saving wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits to local_wcs_cache/
'wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits' -> 'local_wcs_cache/wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits'
wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits exists and is non-empty
Saving wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits to local_wcs_cache/
'wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits' -> 'local_wcs_cache/wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits'
wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits exists and is non-empty
Saving wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits to local_wcs_cache/
'wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits' -> 'local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits'
wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits exists and is non-empty
Saving wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits to local_wcs_cache/
'wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits' -> 'local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits (1st reference image)
verification OK: wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Image size: 941.5'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:39:05.481 -33:59:45.44 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits (1st new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Image size: 940.6'x627.1' 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: 15:39:08.221 -34:00:05.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:39:05.481 -33:59:45.44
Second-epoch image center 15:39:08.221 -34:00:05.53
Angular distance between the image centers 0.0110 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits (2nd new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
Image size: 940.5'x627.1' 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: 15:39:07.431 -34:00:39.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:39:05.481 -33:59:45.44
Second-epoch image center 15:39:07.431 -34:00:39.70
Angular distance between the image centers 0.0165 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 15:39:08.221 -34:00:05.53
Second-epoch second image center 15:39:07.431 -34:00:39.70
Angular distance between the image centers 0.00988 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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits &> /tmp/tmp.IF2qs78Dm1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits &> /tmp/tmp.JIWfC3JYMU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits &> /tmp/tmp.nTt8s0MkB0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits &> /tmp/tmp.Pr6cgccy60
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits and wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits and wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat
Found non-empty wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits and wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat
The reference image (wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits) and catalog (wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat) found
'wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat' -> 'wcsmag.cat'
Read 7114 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.4099 to 244.4457 deg, Dec -39.4422 to -28.0332 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 224.4099 to 244.4457 deg, Dec -39.4422 to -28.0332 deg
Loaded 10950 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): 5601 out of 5758 total matches.
Matched with Tycho-2 5758 out of 7114 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.637500
a=0.000000 b=1.000000 c=22.637500
From vast_summary.log: estimated ref. image limiting mag.: -8.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.16
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7114 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.4099 to 244.4457 deg, Dec -39.4422 to -28.0332 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 224.4099 to 244.4457 deg, Dec -39.4422 to -28.0332 deg
Loaded 10950 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): 5601 out of 5758 total matches.
Matched with Tycho-2 5758 out of 7114 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits (aperture=6.2)
Read 5203 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.8428 to 244.7163 deg, Dec -39.2748 to -28.4901 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 244.7163 deg, Dec -39.2748 to -28.4901 deg
Loaded 10256 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): 4327 out of 4402 total matches.
Matched with Tycho-2 4402 out of 5203 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits (aperture=6.3)
____ 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:
2.3 pix Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
2.5 pix Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
4.1 pix fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
4.1 pix fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
2.3 pix wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
2.5 pix wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
Limiting magnitude estimates:
14.2 mag. Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
13.7 mag. Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
12.5 mag. fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
12.5 mag. fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
All-image limiting magnitude estimate: 12.5 (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.IF2qs78Dm1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits' -> 'wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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=539, bad_region=0, passed=7114
Got 7114 stars (including 6567 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 7114 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.0)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 7015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 311 (Dec -39.4 to -28.0)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7015 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 7014 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits N_match=959 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.400 sigma_q2_arcsec=0.490 sigma_q3_arcsec=0.436 sigma_q4_arcsec=0.466 n_q1=257 n_q2=216 n_q3=212 n_q4=274 worst_quadrant_to_overall_ratio=1.089
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits -region wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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.JIWfC3JYMU (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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits' -> 'wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_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=287, bad_region=0, passed=5203
Got 5203 stars (including 4912 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 5203 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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(), 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: 958 matched stars entering correct_measured_positions(), 5103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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(), 5104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 5104 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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits N_match=958 sigma_overall_arcsec=0.576 sigma_q1_arcsec=0.506 sigma_q2_arcsec=0.897 sigma_q3_arcsec=0.621 sigma_q4_arcsec=0.543 n_q1=245 n_q2=214 n_q3=201 n_q4=298 worst_quadrant_to_overall_ratio=1.558
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits -region wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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.nTt8s0MkB0 (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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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_2026-07-06_21-50-16_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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=249, bad_region=0, passed=1905
Got 1905 stars (including 1656 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 1905 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 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(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 1882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 311 (Dec -39.4 to -28.0)
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(), 1879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 1879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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=fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits N_match=958 sigma_overall_arcsec=0.594 sigma_q1_arcsec=0.750 sigma_q2_arcsec=0.908 sigma_q3_arcsec=0.486 sigma_q4_arcsec=0.461 n_q1=228 n_q2=203 n_q3=224 n_q4=303 worst_quadrant_to_overall_ratio=1.529
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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.Pr6cgccy60 (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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_21-51-02_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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=242, bad_region=0, passed=1991
Got 1991 stars (including 1747 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 1991 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (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 0.010450 (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 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(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 1962 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 252 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(), 1963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 1963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits N_match=957 sigma_overall_arcsec=0.591 sigma_q1_arcsec=0.734 sigma_q2_arcsec=0.874 sigma_q3_arcsec=0.459 sigma_q4_arcsec=0.481 n_q1=228 n_q2=209 n_q3=218 n_q4=302 worst_quadrant_to_overall_ratio=1.478
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits sigma_overall=0.450 worst_q_ratio=1.089
ref2=Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits sigma_overall=0.576 worst_q_ratio=1.558
new1=fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits sigma_overall=0.594 worst_q_ratio=1.529
new2=fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits sigma_overall=0.591 worst_q_ratio=1.478
reference average sigma_overall=0.513 worst_q_ratio=1.3235
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239_astrometric_residuals.png (959 matched stars from wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.42 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001_astrometric_residuals.png (958 matched stars from wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.54 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000_astrometric_residuals.png (958 matched stars from wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001_astrometric_residuals.png (957 matched stars from wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.58 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits'
Saving fully-calibrated image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20211_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 20211_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:25:47.62 -36:13:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20118_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 20118_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:53:28.82 -36:17:53.2 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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.cat to cache
SExtractor catalog cache: saved Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Creating symlink local_wcs_cache/wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
Creating symlink local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Creating symlink local_wcs_cache/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits exists and is non-empty
wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits exists and is non-empty
wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits exists and is non-empty
wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits (1st reference image)
verification OK: wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Image size: 941.5'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 15:39:05.481 -33:59:45.44 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits (1st new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Image size: 940.6'x627.1' 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: 15:39:08.221 -34:00:05.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:39:05.481 -33:59:45.44
Second-epoch image center 15:39:08.221 -34:00:05.53
Angular distance between the image centers 0.0110 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits (2nd new image)
verification OK: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
Image size: 940.5'x627.1' 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: 15:39:07.431 -34:00:39.70 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:39:05.481 -33:59:45.44
Second-epoch image center 15:39:07.431 -34:00:39.70
Angular distance between the image centers 0.0165 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 15:39:08.221 -34:00:05.53
Second-epoch second image center 15:39:07.431 -34:00:39.70
Angular distance between the image centers 0.00988 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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits &> /tmp/tmp.SfCClYOWqQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits &> /tmp/tmp.vgnZ03rpg0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits &> /tmp/tmp.T8bsDr2sDI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits &> /tmp/tmp.KyOSfHgPQ7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits and wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits and wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat
Found non-empty wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits and wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat
The reference image (wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits) and catalog (wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat) found
'wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat' -> 'wcsmag.cat'
Read 70289 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.3696 to 244.4457 deg, Dec -39.4764 to -27.9540 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 224.3696 to 244.4457 deg, Dec -39.4764 to -27.9540 deg
Loaded 11081 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): 7807 out of 8626 total matches.
Matched with Tycho-2 8626 out of 70289 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.435700
a=0.000000 b=1.000000 c=22.435700
From vast_summary.log: estimated ref. image limiting mag.: -8.13
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 70289 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.3696 to 244.4457 deg, Dec -39.4764 to -27.9540 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 224.3696 to 244.4457 deg, Dec -39.4764 to -27.9540 deg
Loaded 11081 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): 7807 out of 8626 total matches.
Matched with Tycho-2 8626 out of 70289 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits (aperture=4.5)
Read 47285 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 224.7645 to 244.7886 deg, Dec -39.2834 to -28.4769 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 224.7645 to 244.7886 deg, Dec -39.2834 to -28.4769 deg
Loaded 10340 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): 8144 out of 8674 total matches.
Matched with Tycho-2 8674 out of 47285 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits:
Forced-photometry filter: calibrated wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits -> calib.txt_param_ref_wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits (aperture=4.8)
____ 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:
2.1 pix Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
2.4 pix Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
3.4 pix fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
3.4 pix fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
2.1 pix wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
2.4 pix wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
Limiting magnitude estimates:
14.3 mag. Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
13.8 mag. Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
12.7 mag. fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
12.7 mag. fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.SfCClYOWqQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits' -> 'wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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=10, blended=3491, bad_region=4, passed=70279
Got 70279 stars (including 66697 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat
util/solve_plate_with_UCAC5 got 70279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 312 (Dec -39.5 to -28.0)
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(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 69314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 252 to 312 (Dec -39.5 to -28.0)
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(), 69315 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 69314 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits N_match=958 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.366 sigma_q2_arcsec=0.492 sigma_q3_arcsec=0.395 sigma_q4_arcsec=0.478 n_q1=260 n_q2=227 n_q3=215 n_q4=256 worst_quadrant_to_overall_ratio=1.125
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits -region wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.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.vgnZ03rpg0 (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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits 572.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits' -> 'wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
Checking if the catalog wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat corresponding to the image wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits
WCS catalog name: wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_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=1840, bad_region=0, passed=47285
Got 47285 stars (including 45378 good ones) from the SExtractor catalog wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 47285 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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
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(), 46474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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(), 46474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 46474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits N_match=957 sigma_overall_arcsec=0.575 sigma_q1_arcsec=0.497 sigma_q2_arcsec=0.765 sigma_q3_arcsec=0.522 sigma_q4_arcsec=0.547 n_q1=248 n_q2=217 n_q3=187 n_q4=305 worst_quadrant_to_overall_ratio=1.330
The image catalog is written to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits -region wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.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.T8bsDr2sDI (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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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_2026-07-06_21-50-16_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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=656, bad_region=1, passed=14620
Got 14620 stars (including 13947 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat
util/solve_plate_with_UCAC5 got 14620 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 311 (Dec -39.4 to -28.0)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 14415 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 252 to 311 (Dec -39.4 to -28.0)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 14417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 14417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits N_match=952 sigma_overall_arcsec=0.573 sigma_q1_arcsec=0.758 sigma_q2_arcsec=0.929 sigma_q3_arcsec=0.457 sigma_q4_arcsec=0.467 n_q1=201 n_q2=189 n_q3=232 n_q4=330 worst_quadrant_to_overall_ratio=1.623
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_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.KyOSfHgPQ7 (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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
WCS_IMAGE_NAME=wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
WCS-calibrated image found: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
Checking if the catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat corresponding to the image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_21-51-02_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits
WCS catalog name: wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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=2, blended=587, bad_region=0, passed=15354
Got 15354 stars (including 14745 good ones) from the SExtractor catalog wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat
util/solve_plate_with_UCAC5 got 15354 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (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 0.010450 (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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15127 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 252 to 311 (Dec -39.4 to -28.0)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 15126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits N_match=952 sigma_overall_arcsec=0.567 sigma_q1_arcsec=0.684 sigma_q2_arcsec=0.854 sigma_q3_arcsec=0.492 sigma_q4_arcsec=0.485 n_q1=194 n_q2=194 n_q3=232 n_q4=332 worst_quadrant_to_overall_ratio=1.505
The image catalog is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits -region wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_21-50-16_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-50-16_20.00sec_0.00C_LIGHTs_0000.fits
Saving fully-calibrated image wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-07-06_CI_Lup-01-Q1b1x1_215142_TTUQ1b1x1_1072691_11yz6A6B/wcs_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_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_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits at 15:36:45.61 -28:51:33.6: 11.40 +/- 0.01 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits at 16:05:19.73 -31:27:26.3: 11.74 +/- 0.03 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits at 15:22:13.82 -32:12:18.9: 11.51 +/- 0.02 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits at 16:05:19.73 -31:27:26.3: 11.60 +/- 0.03 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits at 15:36:45.61 -28:51:33.6: 11.32 +/- 0.02 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits at 15:22:13.82 -32:12:18.9: 11.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.67 +/- 0.02
Forced photometry reference-image weighted average: 11.38 +/- 0.01
Forced photometry filter REJECTED candidate at 16:05:19.73 -31:27:26.3: ref_mag=11.67 +/- 0.02 new_mean_mag=11.7251 delta=-0.05 (need > 0.90)
Forced photometry reference-image weighted average: 11.41 +/- 0.02
Forced photometry filter REJECTED candidate at 15:36:45.61 -28:51:33.6: ref_mag=11.38 +/- 0.01 new_mean_mag=11.6040 delta=-0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:22:13.82 -32:12:18.9: ref_mag=11.41 +/- 0.02 new_mean_mag=11.5266 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits at 15:18:02.49 -37:50:20.5: 11.97 +/- 0.03 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-04-16_02-36-05_20.00sec_-5.00C_LIGHTs_0239.fits at 15:44:35.48 -37:59:29.0: 12.86 +/- 0.06 detection
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits at 15:18:02.49 -37:50:20.5: 12.10 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.01 +/- 0.03
Forced photometry on wcs_Lup-01-Q1b1x1_2026-05-19_00-35-19_20.00sec_5.00C_LIGHT_0001.fits at 15:44:35.48 -37:59:29.0: 12.97 +/- 0.10 detection
Forced photometry filter KEPT candidate at 15:18:02.49 -37:50:20.5: ref_mag=12.01 +/- 0.03 new_mean_mag=11.0387 delta=0.97 (need > 0.90)
Forced photometry reference-image weighted average: 12.89 +/- 0.05
Forced photometry filter KEPT candidate at 15:44:35.48 -37:59:29.0: ref_mag=12.89 +/- 0.05 new_mean_mag=11.7521 delta=1.14 (need > 0.90)
Adding exclusion_list_local.txt__out06928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09436.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 82347_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 82347_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 82348_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 82348_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 82352_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 82352_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:51:06.85 -31:35:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82362_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 82362_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
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Considering the candidate 82410_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 82410_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:24:02.27 -36:59:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82451_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 82451_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:40:09.78 -31:13:22.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 82472_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 82472_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:30:44.40 -38:20:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81335_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 81335_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:26:26.67 -38:06:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28956_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 28956_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:55:42.18 -35:05:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16126_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 16126_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 16:09:07.83 -37:06:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14536_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 14536_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:36:25.57 -37:07:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03142_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 03142_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:33:17.02 -38:42:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65243_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 65243_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:13:12.08 -31:14:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25975_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 25975_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:13:13.34 -34:51:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35279_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 35279_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:36:35.33 -33:50:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81396_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 81396_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:55:38.19 -29:15:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81338_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 81338_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:01:10.19 -36:01:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06928_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
Preparing report for the candidate 06928_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
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Considering the candidate 80886_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 80886_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:38:51.04 -35:44:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26709_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 26709_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:40:11.39 -35:15:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19295_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 19295_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:25:47.62 -36:13:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19068_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 19068_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:18:04.33 -36:03:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19358_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 19358_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks
**** FOUND 15:53:08.15 -36:34:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09436_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
Preparing report for the candidate 09436_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
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Considering the candidate 58877_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001
The candidate 58877_fd_Lup-01-Q1b1x1_2026-07-06_21-51-02_20.00sec_-0.00C_LIGHTs_0001 did not pass the final checks