This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT
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 08 09.3988 2461261.8988 12.94 05:28:26.66 +13:33:51.0
191.01426 -11.51085 galactic Ori Second-epoch detections are separated by 1.8" and 9.5 pix
The object was found in VSX 3" NSVS J0528268+133349
Type: L:
# Max. Min./Amp. JD0 Period
11.465 R1 Y 0.453 R1 234.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:28:26.66 +13:33:51.0: 13.91 +/- 0.04 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:28:26.66 +13:33:51.0: 13.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 08 09.3988* 05 28 26.66 +13 33 51.0 12.9 U Ori 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
NSVS J0528268+133349,2461261.8988,12.94,0.05,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
NSVS J0528268+133349 20260809.3988 12.94CV 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 08 09.3988 2461261.8988 12.11 05:24:02.69 +10:55:10.8
192.73764 -13.81773 galactic Ori Second-epoch detections are separated by 0.1" and 9.5 pix
The object was found in VSX 3" ASASSN-V J052402.83+105508.9
Type: L
# Max. Min./Amp. JD0 Period
13.630 V 14.090 V
The object was not found in astcheck.
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:24:02.69 +10:55:10.8: 13.06 +/- 0.02 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:24:02.69 +10:55:10.8: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
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 08 09.3988* 05 24 02.69 +10 55 10.8 12.1 U Ori 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
ASASSN-V J052402.83+105508.9,2461261.8988,12.11,0.05,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
ASASSN-V J052402.83+105508.9 20260809.3988 12.11CV 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 08 09.3988 2461261.8988 12.79 05:30:01.90 +12:13:12.0
192.38990 -11.88748 galactic Ori Second-epoch detections are separated by 4.7" and 8.9 pix
The object was found in VSX 2" V0370 Ori
Type: INSB
# Max. Min./Amp. JD0 Period
13.700 pg 16.500 pg K7ea
The object was not found in astcheck.
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:30:01.90 +12:13:12.0: 14.05 +/- 0.05 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:30:01.90 +12:13:12.0: 13.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin 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 08 09.3988* 05 30 01.90 +12 13 12.0 12.8 U Ori 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
V0370 Ori,2461261.8988,12.79,0.05,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
V0370 Ori 20260809.3988 12.79CV 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: 2461032.79071524 23.12.2025 06:58:27.797 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
First image: 2461032.79071524 23.12.2025 06:58:27.797 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Last image: 2461261.89925737 09.08.2026 09:34:45.837 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 10055
Objects passed selection criteria: 9997
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 8803.75
Average stars matched: 7924.25 (90.0099 %)
Memory usage VmPeak: 240388 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 9 05:26:57 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: 2461032.79071524 23.12.2025 06:58:27.797 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
First image: 2461032.79071524 23.12.2025 06:58:27.797 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Last image: 2461261.89925737 09.08.2026 09:34:45.837 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 31
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 18 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 75704
Objects passed selection criteria: 75520
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 67205.5
Average stars matched: 60206.5 (89.5857 %)
Memory usage VmPeak: 502532 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 6 15:05:04 CDT 2026
VaST build number 1.0rc89-190-gdf2934b0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 9 05:27:53 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
SExtractor catalog cache: saved Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.cat to cache
SExtractor catalog cache: saved Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.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/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.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: 2461261.89843671
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_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits exists and is non-empty
Saving wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits to local_wcs_cache/
'wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits' -> 'local_wcs_cache/wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits'
wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits exists and is non-empty
Saving wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits to local_wcs_cache/
'wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits' -> 'local_wcs_cache/wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits'
wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits exists and is non-empty
Saving wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits to local_wcs_cache/
'wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits' -> 'local_wcs_cache/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits'
wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits exists and is non-empty
Saving wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits to local_wcs_cache/
'wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits' -> 'local_wcs_cache/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits (1st reference image)
verification OK: wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:20:07.226 +14:00:41.44 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits (1st new image)
verification OK: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Image size: 940.9'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:19:59.931 +14:00:16.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:20:07.226 +14:00:41.44
Second-epoch image center 05:19:59.931 +14:00:16.59
Angular distance between the image centers 0.0303 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits (2nd new image)
verification OK: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Image size: 940.7'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:19:57.134 +14:00:53.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:20:07.226 +14:00:41.44
Second-epoch image center 05:19:57.134 +14:00:53.36
Angular distance between the image centers 0.0409 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 05:19:59.931 +14:00:16.59
Second-epoch second image center 05:19:57.134 +14:00:53.36
Angular distance between the image centers 0.01524 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits &> /tmp/tmp.NuIJ0z7Uwh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits &> /tmp/tmp.EnJ6VlvvZZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits &> /tmp/tmp.fpjt52wBz6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits &> /tmp/tmp.N7u0iGrUH6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.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_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits and wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits and wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
Found non-empty wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits and wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
The reference image (wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits) and catalog (wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat) found
'wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat' -> 'wcsmag.cat'
Read 18778 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.7748 to 88.3498 deg, Dec +8.6481 to +19.2997 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 71.7748 to 88.3498 deg, Dec 8.6481 to 19.2997 deg
Loaded 8940 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): 6904 out of 7673 total matches.
Matched with Tycho-2 7673 out of 18778 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.977900
a=0.000000 b=1.000000 c=22.977900
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 18778 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.7748 to 88.3498 deg, Dec +8.6481 to +19.2997 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 71.7748 to 88.3498 deg, Dec 8.6481 to 19.2997 deg
Loaded 8940 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): 6904 out of 7673 total matches.
Matched with Tycho-2 7673 out of 18778 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Forced-photometry filter: calibrated wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits -> calib.txt_param_ref_wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits (aperture=6.0)
Read 19240 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.5715 to 88.1444 deg, Dec +8.4866 to +19.3515 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 71.5715 to 88.1444 deg, Dec 8.4866 to 19.3515 deg
Loaded 8970 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): 6863 out of 7649 total matches.
Matched with Tycho-2 7649 out of 19240 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
Forced-photometry filter: calibrated wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
2.1 pix Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
2.4 pix fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
2.4 pix fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Limiting magnitude estimates:
15.4 mag. Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
15.4 mag. Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
13.3 mag. fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
13.3 mag. fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.NuIJ0z7Uwh (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits' -> 'wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WCS_IMAGE_NAME=wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WCS-calibrated image found: wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Checking if the catalog wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits alredy exist and is non-empty...
Catalog wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WCS catalog name: wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1816, bad_region=3005, passed=18778
Got 18778 stars (including 14175 good ones) from the SExtractor catalog wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
util/solve_plate_with_UCAC5 got 18778 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4803 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4746 matched stars entering correct_measured_positions(), 4747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4746 matched stars entering correct_measured_positions(), 16452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4804 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4745 matched stars entering correct_measured_positions(), 16452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4745 matched stars entering correct_measured_positions(), 16452 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4745 stars left (next iteration limit 5220)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits N_match=4745 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.401 sigma_q2_arcsec=0.299 sigma_q3_arcsec=0.265 sigma_q4_arcsec=0.229 n_q1=1785 n_q2=669 n_q3=1584 n_q4=707 worst_quadrant_to_overall_ratio=1.267
The image catalog is written to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits -region wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EnJ6VlvvZZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits' -> 'wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
Checking if the catalog wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WCS catalog name: wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1850, bad_region=6689, passed=19240
Got 19240 stars (including 11393 good ones) from the SExtractor catalog wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 19240 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4807 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 4768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 13853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4807 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 13853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4767 matched stars entering correct_measured_positions(), 13853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4767 stars left (next iteration limit 5243)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits N_match=4767 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.307 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.268 n_q1=1357 n_q2=1015 n_q3=1333 n_q4=1062 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits -region wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fpjt52wBz6 (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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
WCS_IMAGE_NAME=wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
WCS-calibrated image found: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Checking if the catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
WCS catalog name: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=245, bad_region=985, passed=4514
Got 4514 stars (including 3330 good ones) from the SExtractor catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat
util/solve_plate_with_UCAC5 got 4514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3196 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3171 matched stars entering correct_measured_positions(), 3172 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3171 matched stars entering correct_measured_positions(), 3743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3198 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3173 matched stars entering correct_measured_positions(), 3743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 3173 matched stars entering correct_measured_positions(), 3743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 3173 stars left (next iteration limit 3488)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3173 robust_rms=6.463 arcsec worst_quadrant_rms=9.864 arcsec
SIP_REFIT: SIP order 3 trial: matched=3173 robust_rms=0.552 arcsec worst_quadrant_rms=0.687 arcsec
SIP_REFIT: SIP order 5 trial: matched=3173 robust_rms=0.508 arcsec worst_quadrant_rms=0.559 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3173 robust_rms_before=1.607 arcsec robust_rms_before_corrected=0.559 arcsec robust_rms_after=0.508 arcsec worst_quadrant_rms_before=0.618 worst_quadrant_rms_after=0.559
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.618 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits N_match=3173 sigma_overall_arcsec=0.557 sigma_q1_arcsec=0.567 sigma_q2_arcsec=0.566 sigma_q3_arcsec=0.545 sigma_q4_arcsec=0.655 n_q1=1036 n_q2=504 n_q3=964 n_q4=669 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits -region wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.N7u0iGrUH6 (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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
WCS_IMAGE_NAME=wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
WCS-calibrated image found: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Checking if the catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
WCS catalog name: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=255, bad_region=997, passed=4568
Got 4568 stars (including 3359 good ones) from the SExtractor catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat
util/solve_plate_with_UCAC5 got 4568 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010452 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3221 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3196 matched stars entering correct_measured_positions(), 3197 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3196 matched stars entering correct_measured_positions(), 3788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3222 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3198 matched stars entering correct_measured_positions(), 3788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 3198 matched stars entering correct_measured_positions(), 3788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 3198 stars left (next iteration limit 3515)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3198 robust_rms=6.667 arcsec worst_quadrant_rms=9.738 arcsec
SIP_REFIT: SIP order 3 trial: matched=3198 robust_rms=0.571 arcsec worst_quadrant_rms=0.732 arcsec
SIP_REFIT: SIP order 5 trial: matched=3198 robust_rms=0.517 arcsec worst_quadrant_rms=0.565 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3198 robust_rms_before=1.580 arcsec robust_rms_before_corrected=0.564 arcsec robust_rms_after=0.517 arcsec worst_quadrant_rms_before=0.644 worst_quadrant_rms_after=0.565
verification OK: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
verification OK: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Image size: 941.3'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:19:57.246 +14:00:51.76 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 4568 stars ###
'wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/correct_sextractor_wcs_catalog_usingxy2sky2627843.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.580 -> 0.517 arcsec)
WCS_QUALITY_DIAG: file=fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits N_match=3198 sigma_overall_arcsec=0.547 sigma_q1_arcsec=0.557 sigma_q2_arcsec=0.598 sigma_q3_arcsec=0.505 sigma_q4_arcsec=0.625 n_q1=1040 n_q2=502 n_q3=973 n_q4=683 worst_quadrant_to_overall_ratio=1.143
The image catalog is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits -region wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits sigma_overall=0.316 worst_q_ratio=1.267
ref2=Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits sigma_overall=0.315 worst_q_ratio=1.106
new1=fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits sigma_overall=0.557 worst_q_ratio=1.175
new2=fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits sigma_overall=0.547 worst_q_ratio=1.143
reference average sigma_overall=0.3155 worst_q_ratio=1.1865
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346_astrometric_residuals.png (4745 matched stars from wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166_astrometric_residuals.png (4767 matched stars from wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448_astrometric_residuals.png (3173 matched stars from wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449_astrometric_residuals.png (3198 matched stars from wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits'
Saving fully-calibrated image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits'
Preparing the HTML report for the field Ori-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23513_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 23513_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:23:58.95 +14:34:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23514_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 23514_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:28:38.48 +15:40:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09020_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 09020_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:22:52.32 +14:35:43.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16567_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 16567_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:35:07.98 +09:56:04.8 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ori-01-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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
SExtractor catalog cache: saved Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.cat to cache
SExtractor catalog cache: saved Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Creating symlink local_wcs_cache/wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.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_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits exists and is non-empty
wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits exists and is non-empty
wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits exists and is non-empty
wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits (1st reference image)
verification OK: wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:20:07.226 +14:00:41.44 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits (1st new image)
verification OK: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Image size: 940.9'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 05:19:59.931 +14:00:16.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:20:07.226 +14:00:41.44
Second-epoch image center 05:19:59.931 +14:00:16.59
Angular distance between the image centers 0.0303 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits (2nd new image)
verification OK: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Image size: 940.7'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 05:19:57.134 +14:00:53.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:20:07.226 +14:00:41.44
Second-epoch image center 05:19:57.134 +14:00:53.36
Angular distance between the image centers 0.0409 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 05:19:59.931 +14:00:16.59
Second-epoch second image center 05:19:57.134 +14:00:53.36
Angular distance between the image centers 0.01524 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits &> /tmp/tmp.Dc7pB1wyUe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits &> /tmp/tmp.NKsJp3pfee
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits &> /tmp/tmp.3kulnBAq6g
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits &> /tmp/tmp.nnCAAsoa0C
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.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_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits and wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits and wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
Found non-empty wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits and wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
The reference image (wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits) and catalog (wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat) found
'wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat' -> 'wcsmag.cat'
Read 133414 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.7535 to 88.3498 deg, Dec +8.6339 to +19.3006 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 71.7535 to 88.3498 deg, Dec 8.6339 to 19.3006 deg
Loaded 8958 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): 5727 out of 7745 total matches.
Matched with Tycho-2 7745 out of 133414 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.848900
a=0.000000 b=1.000000 c=22.848900
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 133414 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.7535 to 88.3498 deg, Dec +8.6339 to +19.3006 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 71.7535 to 88.3498 deg, Dec 8.6339 to 19.3006 deg
Loaded 8958 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): 5727 out of 7745 total matches.
Matched with Tycho-2 7745 out of 133414 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Forced-photometry filter: calibrated wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits -> calib.txt_param_ref_wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits (aperture=4.6)
Read 134593 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 71.5715 to 88.1446 deg, Dec +8.4624 to +19.3542 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 71.5715 to 88.1446 deg, Dec 8.4624 to 19.3542 deg
Loaded 8990 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): 5766 out of 7720 total matches.
Matched with Tycho-2 7720 out of 134593 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
Forced-photometry filter: calibrated wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits -> calib.txt_param_ref_wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
2.0 pix Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
2.2 pix fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
2.2 pix fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Limiting magnitude estimates:
15.5 mag. Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
15.6 mag. Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
13.7 mag. fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
13.7 mag. fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Dc7pB1wyUe (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits' -> 'wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WCS_IMAGE_NAME=wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WCS-calibrated image found: wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
Checking if the catalog wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits alredy exist and is non-empty...
Catalog wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits
WCS catalog name: wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=13989, bad_region=16769, passed=133386
Got 133386 stars (including 103589 good ones) from the SExtractor catalog wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat
util/solve_plate_with_UCAC5 got 133386 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4796 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 4760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 120780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4796 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 120780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 120780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4760 stars left (next iteration limit 5236)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits N_match=4760 sigma_overall_arcsec=0.293 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.295 sigma_q3_arcsec=0.249 sigma_q4_arcsec=0.225 n_q1=1676 n_q2=708 n_q3=1623 n_q4=753 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits -region wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NKsJp3pfee (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits' -> 'wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
Checking if the catalog wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat corresponding to the image wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits
WCS catalog name: wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=13660, bad_region=38072, passed=134571
Got 134571 stars (including 87554 good ones) from the SExtractor catalog wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat
util/solve_plate_with_UCAC5 got 134571 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4799 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 4774 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 104535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.4)
Done reading UCAC5 zone files...
Matched 4799 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 104535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 104535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4774 stars left (next iteration limit 5251)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits N_match=4774 sigma_overall_arcsec=0.297 sigma_q1_arcsec=0.317 sigma_q2_arcsec=0.296 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.258 n_q1=1395 n_q2=956 n_q3=1399 n_q4=1024 worst_quadrant_to_overall_ratio=1.067
The image catalog is written to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits -region wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3kulnBAq6g (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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
WCS_IMAGE_NAME=wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
WCS-calibrated image found: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Checking if the catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
WCS catalog name: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1270, bad_region=5847, passed=34385
Got 34385 stars (including 27498 good ones) from the SExtractor catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat
util/solve_plate_with_UCAC5 got 34385 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4791 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4754 matched stars entering correct_measured_positions(), 4755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4754 matched stars entering correct_measured_positions(), 30070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4793 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4753 matched stars entering correct_measured_positions(), 30070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4753 matched stars entering correct_measured_positions(), 30070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4753 stars left (next iteration limit 5229)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits N_match=4753 sigma_overall_arcsec=0.517 sigma_q1_arcsec=0.526 sigma_q2_arcsec=0.540 sigma_q3_arcsec=0.525 sigma_q4_arcsec=0.577 n_q1=1501 n_q2=704 n_q3=1545 n_q4=1003 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits -region wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nnCAAsoa0C (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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
WCS_IMAGE_NAME=wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
WCS-calibrated image found: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Checking if the catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat corresponding to the image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
WCS catalog name: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1320, bad_region=5962, passed=34694
Got 34694 stars (including 27645 good ones) from the SExtractor catalog wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat
util/solve_plate_with_UCAC5 got 34694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.7'
Seting catalog search parameters based on the expected field of view 940.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013065 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010452 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4795 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4757 matched stars entering correct_measured_positions(), 4758 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4757 matched stars entering correct_measured_positions(), 30279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 30279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 30279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4758 stars left (next iteration limit 5232)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits N_match=4758 sigma_overall_arcsec=0.536 sigma_q1_arcsec=0.534 sigma_q2_arcsec=0.548 sigma_q3_arcsec=0.525 sigma_q4_arcsec=0.588 n_q1=1515 n_q2=708 n_q3=1533 n_q4=1002 worst_quadrant_to_overall_ratio=1.097
The image catalog is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits -region wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-33-34_20.00sec_-0.00C_LIGHT_0448.fits
Saving fully-calibrated image wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.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_2026-08-09_CI_Ori-01-Q2b1x1_052431_TTUQ2b1x1_2587564_EyQYRuiT/wcs_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449.fits
Preparing the HTML report for the field Ori-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:06:33.23 +10:39:22.9: 12.78 +/- 0.02 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:33:56.21 +15:34:07.3: 12.81 +/- 0.02 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:28:26.66 +13:33:51.0: 13.91 +/- 0.04 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:33:56.21 +15:34:07.3: 12.85 +/- 0.02 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:06:33.23 +10:39:22.9: 12.94 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.02
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter REJECTED candidate at 05:33:56.21 +15:34:07.3: ref_mag=12.83 +/- 0.02 new_mean_mag=12.7364 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 05:06:33.23 +10:39:22.9: ref_mag=12.85 +/- 0.01 new_mean_mag=12.7545 delta=0.09 (need > 0.90)
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:24:02.69 +10:55:10.8: 13.06 +/- 0.02 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:28:26.66 +13:33:51.0: 13.99 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.95 +/- 0.03
Forced photometry filter KEPT candidate at 05:28:26.66 +13:33:51.0: ref_mag=13.95 +/- 0.03 new_mean_mag=12.9349 delta=1.01 (need > 0.90)
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:24:02.69 +10:55:10.8: 13.08 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry filter KEPT candidate at 05:24:02.69 +10:55:10.8: ref_mag=13.07 +/- 0.02 new_mean_mag=12.1082 delta=0.96 (need > 0.90)
Forced photometry on wcs_Ori-01-Q2b1x1_2025-12-23_00-58-27_20.00sec_-14.90C_LIGHT_0346.fits at 05:30:01.90 +12:13:12.0: 14.05 +/- 0.05 detection
Forced photometry on wcs_Ori-01-Q2b1x1_2026-01-08_22-38-00_20.00sec_-14.90C_LIGHT_0166.fits at 05:30:01.90 +12:13:12.0: 13.69 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.81 +/- 0.03
Forced photometry filter KEPT candidate at 05:30:01.90 +12:13:12.0: ref_mag=13.81 +/- 0.03 new_mean_mag=12.7775 delta=1.03 (need > 0.90)
Adding exclusion_list_local.txt__out109946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79090.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171190_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 171190_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:09:40.31 +15:34:06.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171203_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 171203_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:35:18.95 +09:54:54.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171227_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 171227_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171240_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 171240_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:05:16.70 +12:46:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171246_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 171246_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171248_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 171248_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:08:39.88 +15:07:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171268_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 171268_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:15:21.90 +15:38:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153932_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 153932_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 04:59:19.11 +15:45:11.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44402_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 44402_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:18:20.34 +16:15:54.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79090_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
Preparing report for the candidate 79090_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 155937_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 155937_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 04:55:05.74 +13:07:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104791_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 104791_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:23:36.97 +12:44:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125355_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 125355_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:13:40.89 +11:59:12.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 109946_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
Preparing report for the candidate 109946_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113171_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 113171_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:23:48.68 +12:54:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18684_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 18684_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:34:41.09 +17:53:16.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66970_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 66970_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:23:58.94 +14:34:47.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51774_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 51774_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:28:38.45 +15:40:54.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65728_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 65728_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:22:52.33 +14:35:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129120_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
Preparing report for the candidate 129120_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67760_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 67760_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:33:54.03 +14:18:19.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111951_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 111951_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:37:04.32 +11:02:06.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100177_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 100177_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks
**** FOUND 05:35:13.15 +10:14:24.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 105022_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449
The candidate 105022_fd_Ori-01-Q2b1x1_2026-08-09_04-34-45_20.00sec_-0.00C_LIGHT_0449 did not pass the final checks