This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.1068* 05 31 56.21 +07 36 47.8 10.2 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
BK Ori,2461158.6068,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
BK Ori 20260428.1068 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 28.1068 2461158.6068 12.94 05:43:47.97 +08:13:08.3
197.66326 -11.01229 galactic Ori Second-epoch detections are separated by 1.5" and 2.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.386 Siegena 1 3 3 13.3 -0 0
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 05:43:47.97 +08:13:08.3: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 05:43:47.97 +08:13:08.3: 15.91 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.1068* 05 43 47.97 +08 13 08.3 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
VARIABLE_NAME,2461158.6068,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260428.1068 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 28.1068* 06 05 44.68 +08 20 58.7 13.0 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
DX Ori,2461158.6068,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DX Ori 20260428.1068 13.04CV 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: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
First image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Last image: 2461158.60714223 28.04.2026 02:34:07.089 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 22583
Objects passed selection criteria: 22471
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: 15446.5
Average stars matched: 14950 (96.7857 %)
Memory usage VmPeak: 126644 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 27 21:42:26 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: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
First image: 2461082.61632350 11.02.2026 02:47:20.350 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Last image: 2461158.60714223 28.04.2026 02:34:07.089 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 45
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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: 177 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 151464
Objects passed selection criteria: 151063
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: 105317
Average stars matched: 101194 (96.0847 %)
Memory usage VmPeak: 1977908 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Apr 21 18:08:25 CDT 2026
VaST build number 1.0rc89-27-g1ba0f777
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 27 21:49:34 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat to cache
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.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: 2461158.60648014
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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits exists and is non-empty
Saving wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits to local_wcs_cache/
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
Saving wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits to local_wcs_cache/
'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits exists and is non-empty
Saving wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits to local_wcs_cache/
'wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits' -> 'local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits'
wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits exists and is non-empty
Saving wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits to local_wcs_cache/
'wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits' -> 'local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (1st reference image)
verification OK: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.4'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: 05:59:57.477 +05:59:33.49 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-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits (1st new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Image size: 941.9'x626.9' 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: 05:59:48.764 +06:03:13.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:57.477 +05:59:33.49
Second-epoch image center 05:59:48.764 +06:03:13.17
Angular distance between the image centers 0.0709 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits (2nd new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.9'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: 05:59:47.826 +06:03:24.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:57.477 +05:59:33.49
Second-epoch image center 05:59:47.826 +06:03:24.95
Angular distance between the image centers 0.0757 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 05:59:48.764 +06:03:13.17
Second-epoch second image center 05:59:47.826 +06:03:24.95
Angular distance between the image centers 0.00508 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.Ga6HtMC4n8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.8flKu8bdmm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits &> /tmp/tmp.D9GvcdVdup
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits &> /tmp/tmp.jfd3srAvOK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
The reference image (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits) and catalog (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat) found
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat' -> 'wcsmag.cat'
Read 23947 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9166 to 97.9247 deg, Dec +0.5857 to +11.3175 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 81.9166 to 97.9247 deg, Dec 0.5857 to 11.3175 deg
Loaded 13837 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): 10462 out of 11606 total matches.
Matched with Tycho-2 11606 out of 23947 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.904216
a=0.000000 b=1.000000 c=22.904216
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.13
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.13
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 23947 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9166 to 97.9247 deg, Dec +0.5857 to +11.3175 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 81.9166 to 97.9247 deg, Dec 0.5857 to 11.3175 deg
Loaded 13837 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): 10462 out of 11606 total matches.
Matched with Tycho-2 11606 out of 23947 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (aperture=6.3)
Read 23981 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9164 to 97.9130 deg, Dec +0.6082 to +11.3237 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 81.9164 to 97.9130 deg, Dec 0.6082 to 11.3237 deg
Loaded 13818 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): 10487 out of 11619 total matches.
Matched with Tycho-2 11619 out of 23981 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.3 pix Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
3.1 pix fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
3.2 pix fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
2.3 pix wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.3 pix wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Limiting magnitude estimates:
15.1 mag. Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
15.1 mag. Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
13.5 mag. fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
13.5 mag. fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Ga6HtMC4n8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2599, passed=23947
Got 23947 stars (including 21319 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 23947 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 22650 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 22646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 22646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 919 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8flKu8bdmm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.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-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2508, passed=23981
Got 23981 stars (including 21438 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 23981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 22605 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 22606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 22606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 917 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.D9GvcdVdup (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=562, passed=7107
Got 7107 stars (including 6540 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat
util/solve_plate_with_UCAC5 got 7107 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 6988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 6986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 6986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 903 stars left (next iteration limit 993)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits -region wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jfd3srAvOK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=546, passed=7178
Got 7178 stars (including 6626 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat
util/solve_plate_with_UCAC5 got 7178 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 891 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 7059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 7058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 7058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 900 stars left (next iteration limit 990)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits -region wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits'
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits'
Preparing the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out13836.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 31784_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 31784_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:55:04.25 +07:30:09.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13836_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
Preparing report for the candidate 13836_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:31:56.21 +07:36:47.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat to cache
SExtractor catalog cache: saved Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits exists and is non-empty
wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits exists and is non-empty
wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits exists and is non-empty
wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (1st reference image)
verification OK: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Image size: 941.4'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: 05:59:57.477 +05:59:33.49 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-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits (1st new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Image size: 941.9'x626.9' 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: 05:59:48.764 +06:03:13.17 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:59:57.477 +05:59:33.49
Second-epoch image center 05:59:48.764 +06:03:13.17
Angular distance between the image centers 0.0709 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits (2nd new image)
verification OK: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.9'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: 05:59:47.826 +06:03:24.95 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:59:57.477 +05:59:33.49
Second-epoch image center 05:59:47.826 +06:03:24.95
Angular distance between the image centers 0.0757 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 05:59:48.764 +06:03:13.17
Second-epoch second image center 05:59:47.826 +06:03:24.95
Angular distance between the image centers 0.00508 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.tMJRS8UFeB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits &> /tmp/tmp.FNcl2mkcL7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits &> /tmp/tmp.TuMGHLG7YV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits &> /tmp/tmp.N4wWr8blrL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
Found non-empty wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits and wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
The reference image (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits) and catalog (wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat) found
'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat' -> 'wcsmag.cat'
Read 165923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9036 to 97.9252 deg, Dec +0.5721 to +11.3198 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 81.9036 to 97.9252 deg, Dec 0.5721 to 11.3198 deg
Loaded 13865 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): 8472 out of 12113 total matches.
Matched with Tycho-2 12113 out of 165923 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.737308
a=0.000000 b=1.000000 c=22.737308
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 165923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.9036 to 97.9252 deg, Dec +0.5721 to +11.3198 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 81.9036 to 97.9252 deg, Dec 0.5721 to 11.3198 deg
Loaded 13865 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): 8472 out of 12113 total matches.
Matched with Tycho-2 12113 out of 165923 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits (aperture=4.7)
Read 164824 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 81.8915 to 97.9157 deg, Dec +0.5837 to +11.3272 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 81.8915 to 97.9157 deg, Dec 0.5837 to 11.3272 deg
Loaded 13866 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): 8523 out of 12122 total matches.
Matched with Tycho-2 12122 out of 164824 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits via Tycho-2
Forced-photometry filter: calibrated wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -> calib.txt_param_ref_wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 38 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.1 pix Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
2.9 pix fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
3.1 pix fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
2.1 pix wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
2.1 pix wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Limiting magnitude estimates:
15.3 mag. Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
15.3 mag. Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
13.6 mag. fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
13.6 mag. fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 12.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tMJRS8UFeB (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.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-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=21856, passed=165873
Got 165873 stars (including 143783 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 165873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 161438 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 161435 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 161433 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FNcl2mkcL7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.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-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits' -> 'wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
Checking if the catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat corresponding to the image wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits
WCS catalog name: wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=53, blended=21523, passed=164771
Got 164771 stars (including 143001 good ones) from the SExtractor catalog wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 164771 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 160368 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 160368 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 160369 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits -region wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TuMGHLG7YV (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3639, passed=47868
Got 47868 stars (including 44162 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat
util/solve_plate_with_UCAC5 got 47868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 47313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 47313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 900 matched stars entering correct_measured_positions(), 47301 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 900 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits -region wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.N4wWr8blrL (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
WCS_IMAGE_NAME=wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
WCS-calibrated image found: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
Checking if the catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat corresponding to the image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
WCS catalog name: wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3498, passed=46196
Got 46196 stars (including 42637 good ones) from the SExtractor catalog wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat
util/solve_plate_with_UCAC5 got 46196 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 45662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.7)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 45664 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 45665 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 898 stars left (next iteration limit 987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits -region wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-33-09_20.00sec_-5.00C_LIGHTs_0015.fits
Saving fully-calibrated image wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-27_CI_Ori-04-Q1b1x1_213457_TTUQ1b1x1_3050986_WpGXg9Bx/wcs_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016.fits
Preparing the HTML report for the field Ori-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out190248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out109876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191832.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 190237_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190237_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:52:13.83 +09:13:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190247_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190247_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:24:58.87 +08:27:04.7: 12.60 +/- 0.02 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:24:58.87 +08:27:04.7: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
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Considering the candidate 190248_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190248_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:11:47.35 +06:01:22.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 190251_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190251_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:31:32.40 +08:37:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190252_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190252_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:22:16.63 +08:48:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190255_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190255_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:52:20.54 +07:17:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190256_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190256_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:14:22.38 +07:41:01.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)
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Considering the candidate 190272_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190272_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:31:31.05 +09:13:01.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 190628_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190628_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:34:56.71 +11:04:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 0.473 3339819728182624896 083.73615971068 +11.07911638924 10.5559 9.4584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190648_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190648_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:29:12.64 +00:51:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190862_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190862_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 190898_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 190898_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:31:31.26 +10:00:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.641 3327297836931416448 097.88070951819 +10.00238992715 11.2889 10.1390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191126_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191126_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:30:24.56 +04:10:58.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191257_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191257_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 191357_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191357_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:23:13.20 +03:46:08.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191446_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191446_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:06:23.24 +10:45:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191461_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191461_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 191464_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191464_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:50:22.17 +02:03:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 1.432 3316079038755153152 087.59198980035 +02.05003866835 12.3987 11.7131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191471_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191471_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:42:19.72 +02:19:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.705 3223215278809926656 085.58223144819 +02.32877909413 12.1701 11.2488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191496_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191496_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 191520_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191520_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:50:23.33 +02:02:39.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191535_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191535_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:54:16.45 +10:33:30.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191538_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191538_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:46:34.05 +01:11:37.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191550_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191550_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:31:31.97 +09:19:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.807 3327190634548889472 097.88315212046 +09.32233446169 12.3547 11.4604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191611_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191611_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:07:30.74 +11:00:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.687 3330254762997242112 091.87675871697 +11.01165296275 12.6619 11.8391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191650_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191650_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:39:33.48 +09:52:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.293 3336448178855134848 084.88916943560 +09.87245266623 12.7573 12.3816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191754_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191754_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-47-20_20.00sec_-15.00C_LIGHT_0032.fits at 06:13:45.03 +03:35:33.4: 13.04 +/- 0.03 detection
Forced photometry on wcs_Ori-04-Q1b1x1_2026-02-10_20-48-29_20.00sec_-15.00C_LIGHT_0033.fits at 06:13:45.03 +03:35:33.4: 13.12 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.08 +/- 0.02
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Considering the candidate 191798_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 191798_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:31:32.45 +09:16:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.209 3327185789825835904 097.88451115549 +09.26740553085 13.0811 12.6029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191832_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
Preparing report for the candidate 191832_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
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Considering the candidate 192142_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 192142_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 192145_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 192145_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 192220_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 192220_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 99813_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 99813_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:20:57.41 +07:51:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103306_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 103306_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:26:00.90 +08:03:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79779_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 79779_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 06:14:28.78 +06:47:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 2.453 3325068199150067584 093.61926037718 +06.78424556075 13.3771 13.0786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 45229_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 45229_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks
**** FOUND 05:47:51.61 +04:25:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102420_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016
The candidate 102420_fd_Ori-04-Q1b1x1_2026-04-27_21-34-07_20.00sec_-4.90C_LIGHTs_0016 did not pass the final checks