This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE
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 04 23.2751 2461153.7751 12.44 10:29:33.57 +26:08:01.2
206.51265 58.38317 galactic Leo Second-epoch detections are separated by 0.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.416 Vaticana -2 0 2 12.4 -0 0
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits at 10:29:33.57 +26:08:01.2: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits at 10:29:33.57 +26:08:01.2: 16.01 +/- 99.00 upperlimit
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 LiteSNAD ZTF viewer
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!
TCP 2026 04 23.2751* 10 29 33.57 +26 08 01.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7751,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2751 12.44CV 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 04 23.2751 2461153.7751 13.74 10:04:42.86 +18:14:12.4
217.00133 50.71512 galactic Leo Second-epoch detections are separated by 0.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.161 Athor -0 0 0 14.0 -0 0
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits at 10:04:42.86 +18:14:12.4: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits at 10:04:42.86 +18:14:12.4: 16.15 +/- 99.00 upperlimit
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 LiteSNAD ZTF viewer
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!
TCP 2026 04 23.2751* 10 04 42.86 +18 14 12.4 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7751,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2751 13.74CV 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 04 23.2751 2461153.7751 13.88 10:28:46.04 +24:24:19.8
209.65620 57.86949 galactic Leo Second-epoch detections are separated by 0.5" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.508 Princetonia -1 0 1 13.9 0 0
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits at 10:28:46.04 +24:24:19.8: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits at 10:28:46.04 +24:24:19.8: 16.09 +/- 99.00 upperlimit
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 LiteSNAD ZTF viewer
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!
TCP 2026 04 23.2751* 10 28 46.04 +24 24 19.8 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461153.7751,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260423.2751 13.88CV 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: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
First image: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Last image: 2461153.77537640 23.04.2026 06:36:22.521 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6383
Objects passed selection criteria: 6350
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 4518.5
Average stars matched: 4194.25 (92.8239 %)
Memory usage VmPeak: 112104 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 01:46:04 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: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
First image: 2461093.76950778 22.02.2026 06:27:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Last image: 2461153.77537640 23.04.2026 06:36:22.521 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 15 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): 32534
Objects passed selection criteria: 32442
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 24813.8
Average stars matched: 22961 (92.5334 %)
Memory usage VmPeak: 133372 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 23 01:47:47 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.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/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.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: 2461153.77472896
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits'
wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits'
wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits'
wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Image size: 937.6'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:09:07.513 +22:03:31.11 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:20.714 +21:58:57.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:20.714 +21:58:57.41
Angular distance between the image centers 0.0915 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:22.896 +21:59:34.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:22.896 +21:59:34.75
Angular distance between the image centers 0.0886 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 10:09:20.714 +21:58:57.41
Second-epoch second image center 10:09:22.896 +21:59:34.75
Angular distance between the image centers 0.01337 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.jRJiTZD80L
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.JebVczDC6T
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits &> /tmp/tmp.GEyTlYSmqF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits &> /tmp/tmp.Bh8PFpZouT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat' -> 'wcsmag.cat'
Read 7416 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6263 to 161.4713 deg, Dec +15.9835 to +27.7570 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 143.6263 to 161.4713 deg, Dec 15.9835 to 27.7570 deg
Loaded 5159 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): 3609 out of 3783 total matches.
Matched with Tycho-2 3783 out of 7416 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.939489
a=0.000000 b=1.000000 c=22.939489
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7416 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6263 to 161.4713 deg, Dec +15.9835 to +27.7570 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 143.6263 to 161.4713 deg, Dec 15.9835 to 27.7570 deg
Loaded 5159 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): 3609 out of 3783 total matches.
Matched with Tycho-2 3783 out of 7416 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits (aperture=6.5)
Read 7467 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6270 to 161.4850 deg, Dec +15.9836 to +27.7800 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 143.6270 to 161.4850 deg, Dec 15.9836 to 27.7800 deg
Loaded 5181 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): 3597 out of 3782 total matches.
Matched with Tycho-2 3782 out of 7467 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
2.4 pix Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
2.5 pix fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
2.6 pix fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
2.4 pix wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
2.4 pix wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Limiting magnitude estimates:
15.4 mag. Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
15.4 mag. Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
14.7 mag. fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
14.6 mag. fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jRJiTZD80L (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=459, passed=7416
Got 7416 stars (including 6953 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 7416 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 7279 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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 7278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 7278 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 901 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JebVczDC6T (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=475, passed=7467
Got 7467 stars (including 6987 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 7467 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 7338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 7338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 7339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 898 stars left (next iteration limit 987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GEyTlYSmqF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=306, passed=4438
Got 4438 stars (including 4127 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 4438 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 4377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 4377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 4377 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Bh8PFpZouT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=264, passed=3973
Got 3973 stars (including 3704 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 3973 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 3907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 902 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 3908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 3908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 901 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits'
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits (1st reference image)
verification OK: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Image size: 937.6'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 10:09:07.513 +22:03:31.11 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:20.714 +21:58:57.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:20.714 +21:58:57.41
Angular distance between the image centers 0.0915 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:22.896 +21:59:34.75 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:07.513 +22:03:31.11
Second-epoch image center 10:09:22.896 +21:59:34.75
Angular distance between the image centers 0.0886 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 10:09:20.714 +21:58:57.41
Second-epoch second image center 10:09:22.896 +21:59:34.75
Angular distance between the image centers 0.01337 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.9Fg2ZF1Cug
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits &> /tmp/tmp.bY5ZusreQb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits &> /tmp/tmp.DADStVKoxw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits &> /tmp/tmp.GjfXZ79BYc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.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_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits and wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat' -> 'wcsmag.cat'
Read 36419 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6171 to 161.4713 deg, Dec +15.9835 to +27.7791 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 143.6171 to 161.4713 deg, Dec 15.9835 to 27.7791 deg
Loaded 5179 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): 3446 out of 3795 total matches.
Matched with Tycho-2 3795 out of 36419 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.820111
a=0.000000 b=1.000000 c=22.820111
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36419 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6171 to 161.4713 deg, Dec +15.9835 to +27.7791 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 143.6171 to 161.4713 deg, Dec 15.9835 to 27.7791 deg
Loaded 5179 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): 3446 out of 3795 total matches.
Matched with Tycho-2 3795 out of 36419 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits (aperture=5.1)
Read 36194 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.6162 to 161.4850 deg, Dec +15.9836 to +27.7972 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 143.6162 to 161.4850 deg, Dec 15.9836 to 27.7972 deg
Loaded 5189 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): 3428 out of 3794 total matches.
Matched with Tycho-2 3794 out of 36194 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits (aperture=5.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
2.3 pix Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
2.2 pix fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
2.3 pix fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
2.3 pix wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
2.3 pix wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Limiting magnitude estimates:
15.6 mag. Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
15.6 mag. Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
14.9 mag. fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
14.8 mag. fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.9Fg2ZF1Cug (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=1750, passed=36394
Got 36394 stars (including 34600 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 36394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 35738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 35738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 897 matched stars entering correct_measured_positions(), 35738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 897 stars left (next iteration limit 986)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-27-55_20.00sec_-15.00C_LIGHT_0226.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bY5ZusreQb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1825, passed=36174
Got 36174 stars (including 34311 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 36174 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 35506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 529 to 590 (Dec 16.0 to 27.8)
Done reading UCAC5 zone files...
Matched 893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 35506 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 35507 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 891 stars left (next iteration limit 981)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits -region wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-22_00-28-43_20.00sec_-15.00C_LIGHT_0227.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DADStVKoxw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1132, passed=24166
Got 24166 stars (including 23012 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 24166 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 23752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 23750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 23750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 899 stars left (next iteration limit 988)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GjfXZ79BYc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=839, passed=22074
Got 22074 stars (including 21204 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 22074 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 876 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 21736 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 21740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 21740 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 896 stars left (next iteration limit 985)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits -region wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-35-26_20.00sec_-5.00C_LIGHT_0119.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-23_CI_Leo-02-Q2b1x1_013711_TTUQ2b1x1_3671753_O2xRIMmE/wcs_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120.fits
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54946.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: 3s
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Considering the candidate 51984_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 51984_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 10:12:55.74 +21:38:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.076 628928833001184640 153.23216321450 +21.64128767946 13.0910 12.3910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52969_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
Preparing report for the candidate 52969_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
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Considering the candidate 53448_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 53448_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 09:51:55.82 +24:21:46.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53458_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 53458_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 10:26:52.53 +19:22:41.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53938_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 53938_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 10:06:11.67 +23:48:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54342_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 54342_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 09:51:44.23 +20:10:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54515_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
Preparing report for the candidate 54515_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
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Considering the candidate 54619_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 54619_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 09:59:30.74 +21:17:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.521 629467421899916416 149.87815754837 +21.29967854264 13.7094 13.0742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54702_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 54702_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 10:20:25.26 +25:41:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54946_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
Preparing report for the candidate 54946_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
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Considering the candidate 55172_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 55172_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 10:09:28.65 +18:55:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55182_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 55182_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 10:19:17.26 +20:56:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55312_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 55312_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks
**** FOUND 10:06:02.56 +23:50:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55376_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120
The candidate 55376_fd_Leo-02-Q2b1x1_2026-04-23_01-36-22_20.00sec_-4.90C_LIGHT_0120 did not pass the final checks