This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 06 09.4154 2461200.9154 10.06 02:07:50.98 +27:56:16.7
142.85648 -31.96029 galactic Tri Second-epoch detections are separated by 4.0" and 5.4 pix
The object was found in VSX 2" Z Tri
Type: M
# Max. Min./Amp. JD0 Period
11.200 pg 14.800 pg 2432915.00000 216.100000000000 M2e
The object was not found in astcheck.
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:07:50.98 +27:56:16.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:07:50.98 +27:56:16.7: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
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 06 09.4154* 02 07 50.98 +27 56 16.7 10.1 U Tri 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
Z Tri,2461200.9154,10.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Z Tri 20260609.4154 10.06CV 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 06 09.4154 2461200.9154 11.54 02:19:29.10 +28:04:12.6
145.60057 -30.89679 galactic Tri Second-epoch detections are separated by 0.4" and 5.3 pix
The object was found in VSX 3" AO Tri
Type: SR:
# Max. Min./Amp. JD0 Period
12.500 V 13.800 V 2452929.40000 90.958705000000 M7III
The object was not found in astcheck.
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:29.10 +28:04:12.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:29.10 +28:04:12.6: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.50 +/- 0.01
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 06 09.4154* 02 19 29.10 +28 04 12.6 11.5 U Tri 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
AO Tri,2461200.9154,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AO Tri 20260609.4154 11.54CV 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 06 09.4154 2461200.9154 11.73 02:13:15.75 +33:57:48.6
141.73041 -25.90375 galactic Tri Second-epoch detections are separated by 1.6" and 5.0 pix
The object was found in VSX 2" AN Tri
Type: SR:
# Max. Min./Amp. JD0 Period
12.400 V 13.400 V 183.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:13:15.75 +33:57:48.6: 12.78 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:13:15.75 +33:57:48.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
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 06 09.4154* 02 13 15.75 +33 57 48.6 11.7 U Tri 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
AN Tri,2461200.9154,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AN Tri 20260609.4154 11.73CV 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: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
First image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Last image: 2461200.91566653 09.06.2026 09:58:23.588 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.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.: -7.49
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: 6 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): 9903
Objects passed selection criteria: 9849
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 6558.5
Average stars matched: 6126.75 (93.4169 %)
Memory usage VmPeak: 115392 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 06:36:12 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: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
First image: 2461049.65440406 09.01.2026 03:42:10.511 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Last image: 2461200.91566653 09.06.2026 09:58:23.588 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 29 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): 61316
Objects passed selection criteria: 61131
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: 43104
Average stars matched: 40114.8 (93.065 %)
Memory usage VmPeak: 159452 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 8 11:26:26 CDT 2026
VaST build number 1.0rc89-95-g079870fa
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jun 9 06:39:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.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/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.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: 2461200.91520133
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'
Plate-solving the images
wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits exists and is non-empty
Saving wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits to local_wcs_cache/
'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits'
wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits exists and is non-empty
Saving wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits to local_wcs_cache/
'wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits' -> 'local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits'
wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits exists and is non-empty
Saving wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits'
wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits exists and is non-empty
Saving wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (1st reference image)
verification OK: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Image size: 941.5'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: 02:00:00.720 +29:59:44.33 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_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits (1st new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:05.490 +30:00:57.44 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:05.490 +30:00:57.44
Angular distance between the image centers 0.0266 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits (2nd new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Image size: 939.0'x624.2' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:07.922 +30:00:59.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:07.922 +30:00:59.43
Angular distance between the image centers 0.0333 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 02:00:05.490 +30:00:57.44
Second-epoch second image center 02:00:07.922 +30:00:59.43
Angular distance between the image centers 0.00879 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/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits &> /tmp/tmp.u3kSPW6Rgf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits &> /tmp/tmp.WNTx6aIDJW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits &> /tmp/tmp.lVNL5gsIw2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits &> /tmp/tmp.EKQdNWAG75
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
The reference image (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits) and catalog (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat) found
'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat' -> 'wcsmag.cat'
Read 12225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6045 to 39.6615 deg, Dec +24.4131 to +35.2963 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 20.6045 to 39.6615 deg, Dec 24.4131 to 35.2963 deg
Loaded 8371 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): 6352 out of 6782 total matches.
Matched with Tycho-2 6782 out of 12225 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.922200
a=0.000000 b=1.000000 c=22.922200
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 12225 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6045 to 39.6615 deg, Dec +24.4131 to +35.2963 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 20.6045 to 39.6615 deg, Dec 24.4131 to 35.2963 deg
Loaded 8371 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): 6352 out of 6782 total matches.
Matched with Tycho-2 6782 out of 12225 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (aperture=5.9)
Read 12296 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.6045 to 39.7012 deg, Dec +24.4131 to +35.3109 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 20.6045 to 39.7012 deg, Dec 24.4131 to 35.3109 deg
Loaded 8408 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): 6364 out of 6800 total matches.
Matched with Tycho-2 6800 out of 12296 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits (aperture=6.0)
____ 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:
2.0 pix Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
2.3 pix fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
2.3 pix fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
2.0 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Limiting magnitude estimates:
15.4 mag. Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
15.4 mag. Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
13.9 mag. fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
13.9 mag. fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.2 (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.u3kSPW6Rgf (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=932, passed=12225
Got 12225 stars (including 11278 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 12225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 12063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 12061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 12061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits N_match=955 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.376 sigma_q4_arcsec=0.360 n_q1=207 n_q2=302 n_q3=208 n_q4=238 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WNTx6aIDJW (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=960, passed=12296
Got 12296 stars (including 11323 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 12296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 12127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 572 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 12127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 12127 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits N_match=956 sigma_overall_arcsec=0.293 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.270 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.303 n_q1=208 n_q2=301 n_q3=210 n_q4=237 worst_quadrant_to_overall_ratio=1.218
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.lVNL5gsIw2 (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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=320, passed=4773
Got 4773 stars (including 4449 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 4773 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4710 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 4710 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits N_match=952 sigma_overall_arcsec=0.496 sigma_q1_arcsec=0.506 sigma_q2_arcsec=0.528 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.620 n_q1=224 n_q2=212 n_q3=286 n_q4=230 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits -region wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.EKQdNWAG75 (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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=312, passed=4710
Got 4710 stars (including 4395 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat
util/solve_plate_with_UCAC5 got 4710 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 4658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits N_match=954 sigma_overall_arcsec=0.497 sigma_q1_arcsec=0.468 sigma_q2_arcsec=0.515 sigma_q3_arcsec=0.428 sigma_q4_arcsec=0.602 n_q1=219 n_q2=212 n_q3=288 n_q4=235 worst_quadrant_to_overall_ratio=1.212
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits -region wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits sigma_overall=0.349 worst_q_ratio=1.076
ref2=Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits sigma_overall=0.293 worst_q_ratio=1.218
new1=fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits sigma_overall=0.496 worst_q_ratio=1.250
new2=fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits sigma_overall=0.497 worst_q_ratio=1.212
reference average sigma_overall=0.321 worst_q_ratio=1.147
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113_astrometric_residuals.png (955 matched stars from wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114_astrometric_residuals.png (956 matched stars from wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300_astrometric_residuals.png (952 matched stars from wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301_astrometric_residuals.png (954 matched stars from wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits'
Saving fully-calibrated image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits'
Preparing the HTML report for the field Tri-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:07:50.91 +27:56:14.9: 12.83 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:07:50.91 +27:56:14.9: 12.84 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.01
Forced photometry filter KEPT candidate at 02:07:50.91 +27:56:14.9: ref_mag=12.84 +/- 0.01 new_mean_mag=10.0537 delta=2.78 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20870.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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 20795_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 20795_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:56:47.07 +34:01:08.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20870_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 20870_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:07:50.91 +27:56:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.05, MAG_FAINT_SEARCH_LIMIT=11.03)GAIADR2_OUTPUT=# 0.433 107473451979882496 031.96225723318 +27.93750085601 10.5924 9.4990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Tri-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Creating symlink local_wcs_cache/wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits exists and is non-empty
wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits exists and is non-empty
wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits exists and is non-empty
wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (1st reference image)
verification OK: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Image size: 941.5'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: 02:00:00.720 +29:59:44.33 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_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits (1st new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
Image size: 939.0'x624.3' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:05.490 +30:00:57.44 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:05.490 +30:00:57.44
Angular distance between the image centers 0.0266 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits (2nd new image)
verification OK: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Image size: 939.0'x624.2' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:00:07.922 +30:00:59.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:00:00.720 +29:59:44.33
Second-epoch image center 02:00:07.922 +30:00:59.43
Angular distance between the image centers 0.0333 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 02:00:05.490 +30:00:57.44
Second-epoch second image center 02:00:07.922 +30:00:59.43
Angular distance between the image centers 0.00879 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/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits &> /tmp/tmp.k2VidVu2Sq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits &> /tmp/tmp.Xp7WDvYqGF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits &> /tmp/tmp.YZ9sAWTWp8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits &> /tmp/tmp.crYTcDI41c
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.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_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
Found non-empty wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits and wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
The reference image (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits) and catalog (wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat) found
'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat' -> 'wcsmag.cat'
Read 73246 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5720 to 39.6905 deg, Dec +24.3228 to +35.3067 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 20.5720 to 39.6905 deg, Dec 24.3228 to 35.3067 deg
Loaded 8456 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): 5809 out of 6892 total matches.
Matched with Tycho-2 6892 out of 73246 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.802700
a=0.000000 b=1.000000 c=22.802700
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 73246 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5720 to 39.6905 deg, Dec +24.3228 to +35.3067 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 20.5720 to 39.6905 deg, Dec 24.3228 to 35.3067 deg
Loaded 8456 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): 5809 out of 6892 total matches.
Matched with Tycho-2 6892 out of 73246 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits (aperture=4.6)
Read 72377 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 20.5786 to 39.7012 deg, Dec +24.3308 to +35.3160 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 20.5786 to 39.7012 deg, Dec 24.3308 to 35.3160 deg
Loaded 8467 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): 5844 out of 6896 total matches.
Matched with Tycho-2 6896 out of 72377 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits:
Forced-photometry filter: calibrated wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -> calib.txt_param_ref_wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
2.2 pix fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
2.1 pix fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
1.9 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
2.0 pix wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Limiting magnitude estimates:
15.6 mag. Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
15.6 mag. Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
14.2 mag. fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
14.2 mag. fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.8 (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.k2VidVu2Sq (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=4778, passed=73232
Got 73232 stars (including 68326 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat
util/solve_plate_with_UCAC5 got 73232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 72663 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 72662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 72662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits N_match=955 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.290 sigma_q3_arcsec=0.280 sigma_q4_arcsec=0.261 n_q1=213 n_q2=290 n_q3=215 n_q4=237 worst_quadrant_to_overall_ratio=1.125
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Xp7WDvYqGF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits' -> 'wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS-calibrated image found: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
Checking if the catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat corresponding to the image wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits
WCS catalog name: wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=4568, passed=72360
Got 72360 stars (including 67666 good ones) from the SExtractor catalog wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat
util/solve_plate_with_UCAC5 got 72360 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 71654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 71654 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 71655 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits N_match=955 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.281 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.278 n_q1=215 n_q2=285 n_q3=220 n_q4=235 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits -region wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.YZ9sAWTWp8 (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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1521, passed=31841
Got 31841 stars (including 30272 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat
util/solve_plate_with_UCAC5 got 31841 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 31558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 31557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 31557 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits N_match=950 sigma_overall_arcsec=0.480 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.530 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.579 n_q1=230 n_q2=209 n_q3=277 n_q4=234 worst_quadrant_to_overall_ratio=1.205
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits -region wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.crYTcDI41c (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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat corresponding to the image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1268, passed=31846
Got 31846 stars (including 30543 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat
util/solve_plate_with_UCAC5 got 31846 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 31618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 31619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 31619 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits N_match=949 sigma_overall_arcsec=0.485 sigma_q1_arcsec=0.414 sigma_q2_arcsec=0.529 sigma_q3_arcsec=0.432 sigma_q4_arcsec=0.578 n_q1=228 n_q2=209 n_q3=276 n_q4=236 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits -region wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-57-43_20.00sec_5.00C_LIGHT_0300.fits
Saving fully-calibrated image wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.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_2026-06-09_CI_Tri-01-Q2b1x1_054614_TTUQ2b1x1_1619747_TWmwh7cn/wcs_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301.fits
Preparing the HTML report for the field Tri-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:05:02.71 +27:35:51.1: 12.08 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:03:36.96 +27:29:56.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:11:05.83 +30:07:32.5: 12.40 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:09:22.70 +28:22:11.3: 13.29 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:56:14.52 +27:29:13.7: 12.31 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:44:15.05 +32:43:16.6: 13.58 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:40:57.68 +27:09:50.7: 12.22 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:44:32.47 +33:37:51.9: 13.77 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:20:35.72 +33:31:59.8: 12.83 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:05:02.71 +27:35:51.1: 12.07 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:03:36.96 +27:29:56.6: 12.85 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:11:05.83 +30:07:32.5: 12.39 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry filter REJECTED candidate at 02:05:02.71 +27:35:51.1: ref_mag=12.08 +/- 0.01 new_mean_mag=12.1611 delta=-0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:03:36.96 +27:29:56.6: ref_mag=12.85 +/- 0.01 new_mean_mag=12.8038 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:44:15.05 +32:43:16.6: 13.57 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 02:11:05.83 +30:07:32.5: ref_mag=12.39 +/- 0.01 new_mean_mag=12.4128 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:56:14.52 +27:29:13.7: 12.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.02
Forced photometry filter REJECTED candidate at 01:44:15.05 +32:43:16.6: ref_mag=13.57 +/- 0.02 new_mean_mag=13.5201 delta=0.05 (need > 0.90)
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:40:36.03 +33:18:03.4: 12.85 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 01:56:14.52 +27:29:13.7: ref_mag=12.29 +/- 0.01 new_mean_mag=12.3258 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:40:57.68 +27:09:50.7: 12.19 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.20 +/- 0.01
Forced photometry filter REJECTED candidate at 01:40:57.68 +27:09:50.7: ref_mag=12.20 +/- 0.01 new_mean_mag=12.4333 delta=-0.23 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:09:22.70 +28:22:11.3: 13.31 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.30 +/- 0.02
Forced photometry filter REJECTED candidate at 02:09:22.70 +28:22:11.3: ref_mag=13.30 +/- 0.02 new_mean_mag=13.2343 delta=0.07 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:20:35.72 +33:31:59.8: 12.77 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter REJECTED candidate at 02:20:35.72 +33:31:59.8: ref_mag=12.80 +/- 0.01 new_mean_mag=12.7470 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:44:32.47 +33:37:51.9: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.77 +/- 0.03
Forced photometry filter REJECTED candidate at 01:44:32.47 +33:37:51.9: ref_mag=13.77 +/- 0.03 new_mean_mag=13.9212 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:40:36.03 +33:18:03.4: 12.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter REJECTED candidate at 01:40:36.03 +33:18:03.4: ref_mag=12.83 +/- 0.01 new_mean_mag=12.9231 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:41:38.24 +33:19:30.8: 13.07 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:01:01.67 +29:33:02.1: 13.22 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:58:48.09 +32:51:27.7: 13.40 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:17:54.66 +31:16:19.0: 13.15 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:11:12.02 +30:07:30.2: 13.13 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:43:03.34 +31:01:41.1: 13.59 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:59:35.98 +27:39:28.7: 13.61 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:55:04.16 +27:16:02.8: 13.55 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:51:42.15 +33:45:29.4: 13.63 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:47:49.38 +28:03:20.1: 13.76 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:41:38.24 +33:19:30.8: 13.05 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:58:48.09 +32:51:27.7: 13.37 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.02
Forced photometry reference-image weighted average: 13.39 +/- 0.02
Forced photometry filter REJECTED candidate at 01:41:38.24 +33:19:30.8: ref_mag=13.06 +/- 0.02 new_mean_mag=13.1661 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:58:48.09 +32:51:27.7: ref_mag=13.39 +/- 0.02 new_mean_mag=13.2128 delta=0.17 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:01:01.67 +29:33:02.1: 13.21 +/- 0.03 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:17:54.66 +31:16:19.0: 13.07 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.21 +/- 0.02
Forced photometry filter REJECTED candidate at 02:01:01.67 +29:33:02.1: ref_mag=13.21 +/- 0.02 new_mean_mag=13.1458 delta=0.07 (need > 0.90)
Forced photometry reference-image weighted average: 13.11 +/- 0.02
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:11:12.02 +30:07:30.2: 13.13 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 02:17:54.66 +31:16:19.0: ref_mag=13.11 +/- 0.02 new_mean_mag=13.1186 delta=-0.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.13 +/- 0.02
Forced photometry filter REJECTED candidate at 02:11:12.02 +30:07:30.2: ref_mag=13.13 +/- 0.02 new_mean_mag=13.1319 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:43:03.34 +31:01:41.1: 13.48 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.53 +/- 0.02
Forced photometry filter REJECTED candidate at 01:43:03.34 +31:01:41.1: ref_mag=13.53 +/- 0.02 new_mean_mag=13.3975 delta=0.14 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:59:35.98 +27:39:28.7: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.63 +/- 0.03
Forced photometry filter REJECTED candidate at 01:59:35.98 +27:39:28.7: ref_mag=13.63 +/- 0.03 new_mean_mag=13.5121 delta=0.12 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:55:04.16 +27:16:02.8: 13.56 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.03
Forced photometry filter REJECTED candidate at 01:55:04.16 +27:16:02.8: ref_mag=13.56 +/- 0.03 new_mean_mag=13.4652 delta=0.09 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:51:42.15 +33:45:29.4: 13.71 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter REJECTED candidate at 01:51:42.15 +33:45:29.4: ref_mag=13.67 +/- 0.03 new_mean_mag=13.5706 delta=0.10 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:47:49.38 +28:03:20.1: 13.77 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.76 +/- 0.03
Forced photometry filter REJECTED candidate at 01:47:49.38 +28:03:20.1: ref_mag=13.76 +/- 0.03 new_mean_mag=13.5622 delta=0.20 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:49:52.47 +27:13:35.5: 13.95 +/- 0.05 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 01:50:34.37 +27:57:41.7: 13.64 +/- 0.04 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:07:50.98 +27:56:16.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:19:29.10 +28:04:12.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-42-10_20.00sec_-14.90C_LIGHT_0113.fits at 02:13:15.75 +33:57:48.6: 12.78 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:49:52.47 +27:13:35.5: 13.88 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 01:50:34.37 +27:57:41.7: 13.67 +/- 0.04 detection
Forced photometry filter REJECTED candidate at 01:49:52.47 +27:13:35.5: ref_mag=13.91 +/- 0.03 new_mean_mag=13.8327 delta=0.08 (need > 0.90)
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter REJECTED candidate at 01:50:34.37 +27:57:41.7: ref_mag=13.66 +/- 0.03 new_mean_mag=13.7453 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:07:50.98 +27:56:16.7: 12.99 +/- 0.02 detection
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:19:29.10 +28:04:12.6: 12.50 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.01
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter KEPT candidate at 02:07:50.98 +27:56:16.7: ref_mag=12.99 +/- 0.01 new_mean_mag=10.0653 delta=2.92 (need > 0.90)
Forced photometry filter KEPT candidate at 02:19:29.10 +28:04:12.6: ref_mag=12.50 +/- 0.01 new_mean_mag=11.5392 delta=0.96 (need > 0.90)
Forced photometry on wcs_Tri-01-Q2b1x1_2026-01-08_21-43-02_20.00sec_-14.90C_LIGHT_0114.fits at 02:13:15.75 +33:57:48.6: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.79 +/- 0.01
Forced photometry filter KEPT candidate at 02:13:15.75 +33:57:48.6: ref_mag=12.79 +/- 0.01 new_mean_mag=11.7257 delta=1.06 (need > 0.90)
Adding exclusion_list_local.txt__out08905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70911.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 87328_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 87328_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 87331_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 87331_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 87334_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 87334_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 87337_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 87337_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 87340_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 87340_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 89344_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 89344_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 89465_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 89465_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 89754_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 89754_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:17:06.11 +34:11:30.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 90192_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 90192_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 90365_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 90365_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 90404_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 90404_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 90528_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 90528_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 90851_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 90851_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 90926_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 90926_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 91363_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 91363_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 91495_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 91495_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 91502_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 91502_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:11:28.97 +31:30:21.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91614_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 91614_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 92199_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 92199_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 92305_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 92305_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 92428_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 92428_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 92763_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 92763_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 93318_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 93318_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 94067_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 94067_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
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Considering the candidate 68673_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
Preparing report for the candidate 68673_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
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Considering the candidate 70911_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
Preparing report for the candidate 70911_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
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Considering the candidate 10047_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 10047_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks
**** FOUND 01:56:47.07 +34:01:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08905_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
Preparing report for the candidate 08905_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
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Considering the candidate 12017_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301
The candidate 12017_fd_Tri-01-Q2b1x1_2026-06-09_04-58-23_20.00sec_5.00C_LIGHT_0301 did not pass the final checks