This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG
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 05 15.4088 2461175.9088 13.29 00:01:19.82 +57:20:32.8
116.18603 -4.87154 galactic Cas Second-epoch detections are separated by 2.2" and 6.2 pix
The object was found in VSX 2" ASASSN-V J000119.83+572031.3
Type: SR
# Max. Min./Amp. JD0 Period
14.930 V 15.600 V 2458511.32860 77.263345700000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits at 00:01:19.82 +57:20:32.8: 14.23 +/- 0.07 detection
Forced photometry on wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits at 00:01:19.82 +57:20:32.8: 14.39 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.06
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 05 15.4088* 00 01 19.82 +57 20 32.8 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J000119.83+572031.3,2461175.9088,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J000119.83+572031.3 20260515.4088 13.29CV 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 05 15.4088 2461175.9088 12.65 23:56:18.38 +58:01:21.9
115.66520 -4.06904 galactic Cas Second-epoch detections are separated by 2.0" and 6.0 pix
The object was found in VSX 4" NSVS J2356179+580117
Type: SR
# Max. Min./Amp. JD0 Period
13.323 r Y 0.219 r 2458251.25580 145.872685100000
The object was not found in astcheck.
Forced photometry on wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits at 23:56:18.38 +58:01:21.9: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits at 23:56:18.38 +58:01:21.9: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 13.90 +/- 0.04
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 05 15.4088* 23 56 18.38 +58 01 21.9 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2356179+580117,2461175.9088,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2356179+580117 20260515.4088 12.65CV 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 3
Ref. image: 2461061.56554947 21.01.2026 01:34:13.474 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
First image: 2461061.56554947 21.01.2026 01:34:13.474 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
Last image: 2461175.90907265 15.05.2026 09:48:53.877 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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: 12 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): 24653
Objects passed selection criteria: 24501
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 3
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 3
Average stars detected per image: 19986
Average stars matched: 19808.3 (99.111 %)
Memory usage VmPeak: 129928 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri May 15 04:51:14 CDT 2026
Host name: tau
***** IMAGE PROCESSING ERROR (less than 4 images processed) *****
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461061.56554947 21.01.2026 01:34:13.474 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
First image: 2461061.56554947 21.01.2026 01:34:13.474 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
Last image: 2461175.90907265 15.05.2026 09:48:53.877 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 26
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
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: 52 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): 181794
Objects passed selection criteria: 181124
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 119410
Average stars matched: 110457 (92.5017 %)
Memory usage VmPeak: 1943600 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri May 15 04:56:26 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
SExtractor catalog cache: saved Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat to cache
SExtractor catalog cache: saved Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.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/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
Last image: 2461175.90856797 15.05.2026 09:48:10.273 UTC
ERROR running VaST on the field Cas-02-Q1b1x1 (less than 4 images processed)
exp_start= 21.01.2026 01:34:13.474 exp= 20.000 JD= 2461061.56554947 ap= 6.0 rotation= 0.000 *detected= 30018 *matched= 30018 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
exp_start= 11.02.2026 02:23:50.335 exp= 20.000 JD= 2461082.60000388 ap= 6.1 rotation= -0.178 *detected= 25119 *matched= 24640 status=OK /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
exp_start= 15.05.2026 09:48:10.273 exp= 20.000 JD= 2461175.90856797 ap= 7.6 rotation= 10.813 *detected= 6484 *matched= 145 status=ERROR /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
exp_start= 15.05.2026 09:48:53.877 exp= 20.000 JD= 2461175.90907265 ap= 7.4 rotation= -177.708 *detected= 4821 *matched= 4767 status=OK /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
SExtractor catalog cache: saved Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat to cache
SExtractor catalog cache: saved Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.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: 2461175.90856797
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits exists and is non-empty
NOT SAVING wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits exists and is non-empty
NOT SAVING wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits exists and is non-empty
NOT SAVING wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits exists and is non-empty
NOT SAVING wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits to local_wcs_cache/ as this is the run with default.sex.telephoto_lens_vSTL
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits (1st reference image)
verification OK: wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
Image size: 943.5'x628.6' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 23:59:58.597 +61:59:18.65 J2000 4789.000 3195.000
###################################
The image scale is 5.91"/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_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits (1st new image)
verification OK: wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 23:59:44.728 +62:00:21.71 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:58.597 +61:59:18.65
Second-epoch image center 23:59:44.728 +62:00:21.71
Angular distance between the image centers 0.0323 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits (2nd new image)
verification OK: wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
Image size: 941.4'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 23:59:42.143 +62:00:50.64 J2000 4789.000 3195.000
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###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:58.597 +61:59:18.65
Second-epoch image center 23:59:42.143 +62:00:50.64
Angular distance between the image centers 0.0411 deg.
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###################################
# 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 23:59:44.728 +62:00:21.71
Second-epoch second image center 23:59:42.143 +62:00:50.64
Angular distance between the image centers 0.00949 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/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits &> /tmp/tmp.qm5JBpKjTB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits &> /tmp/tmp.yAaV0UmhOW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits &> /tmp/tmp.XBbgu7R4aw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits &> /tmp/tmp.fukka9fFaE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.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_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits and wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits and wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat
Found non-empty wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits and wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat
The reference image (wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits) and catalog (wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat) found
'wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat' -> 'wcsmag.cat'
Read 212671 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 359.9999 deg, Dec +55.2738 to +67.4144 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 0.0000 to 359.9999 deg, Dec 55.2738 to 67.4144 deg
Loaded 134222 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): 1171 out of 1789 total matches.
Matched with Tycho-2 1789 out of 212671 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.816100
a=0.000000 b=1.000000 c=22.816100
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 212671 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 359.9999 deg, Dec +55.2738 to +67.4144 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 0.0000 to 359.9999 deg, Dec 55.2738 to 67.4144 deg
Loaded 134222 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): 1171 out of 1789 total matches.
Matched with Tycho-2 1789 out of 212671 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits:
Forced-photometry filter: calibrated wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits -> calib.txt_param_ref_wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits (aperture=4.6)
Read 192191 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0000 to 360.0000 deg, Dec +55.2822 to +67.4366 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 0.0000 to 360.0000 deg, Dec 55.2822 to 67.4366 deg
Loaded 134240 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): 11418 out of 16934 total matches.
Matched with Tycho-2 16934 out of 192191 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits:
Forced-photometry filter: calibrated wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits -> calib.txt_param_ref_wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
1.9 pix Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
3.2 pix fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
3.0 pix fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
1.9 pix wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
1.9 pix wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
Limiting magnitude estimates:
15.4 mag. Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
15.2 mag. Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
14.3 mag. fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
14.0 mag. fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qm5JBpKjTB (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits' -> 'wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
WCS-calibrated image found: wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
Checking if the catalog wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits
WCS catalog name: wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=34581, passed=212618
Got 212618 stars (including 177731 good ones) from the SExtractor catalog wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat
util/solve_plate_with_UCAC5 got 212618 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.5'
Seting catalog search parameters based on the expected field of view 943.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013104 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010483 (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
RA wraps around 0/360 boundary: field RA 341.1650 through 0 to 20.0662, gap 20.0662 to 341.1650
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 200391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 341.1693 through 0 to 20.0648, gap 20.0648 to 341.1693
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 200407 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.47"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 204814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.25"
Excluding outliers - 960 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits N_match=960 sigma_overall_arcsec=1.839 sigma_q1_arcsec=1.521 sigma_q2_arcsec=1.513 sigma_q3_arcsec=1.413 sigma_q4_arcsec=1.591 n_q1=175 n_q2=256 n_q3=245 n_q4=284 worst_quadrant_to_overall_ratio=0.865
The image catalog is written to wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits -region wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yAaV0UmhOW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits' -> 'wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
WCS-calibrated image found: wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
Checking if the catalog wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat corresponding to the image wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits
WCS catalog name: wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=49, blended=28937, passed=192142
Got 192142 stars (including 162924 good ones) from the SExtractor catalog wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 192142 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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
RA wraps around 0/360 boundary: field RA 341.2056 through 0 to 20.1629, gap 20.1629 to 341.2056
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 187484 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
RA wraps around 0/360 boundary: field RA 341.2051 through 0 to 20.1627, gap 20.1627 to 341.2051
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 187481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 187484 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits N_match=978 sigma_overall_arcsec=0.457 sigma_q1_arcsec=0.531 sigma_q2_arcsec=0.428 sigma_q3_arcsec=0.459 sigma_q4_arcsec=0.403 n_q1=192 n_q2=254 n_q3=245 n_q4=287 worst_quadrant_to_overall_ratio=1.162
The image catalog is written to wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits -region wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XBbgu7R4aw (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_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.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_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
Checking if the catalog wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
WCS catalog name: wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=3513, passed=41894
Got 41894 stars (including 38350 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat
util/solve_plate_with_UCAC5 got 41894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 340.9353 through 0 to 19.5104, gap 19.5104 to 340.9353
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 41266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 340.9340 through 0 to 19.5101, gap 19.5101 to 340.9340
Reading UCAC5 zone files...
Searching UCAC5 zones 728 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 41266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 41266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits N_match=973 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.379 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.646 n_q1=419 n_q2=202 n_q3=323 n_q4=29 worst_quadrant_to_overall_ratio=1.695
The image catalog is written to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits -region wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fukka9fFaE (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_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.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_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
Checking if the catalog wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat corresponding to the image wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
WCS catalog name: wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2749, passed=33632
Got 33632 stars (including 30856 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat
util/solve_plate_with_UCAC5 got 33632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 340.7969 through 0 to 18.4234, gap 18.4234 to 340.7969
Reading UCAC5 zone files...
Searching UCAC5 zones 731 to 788 (Dec 56.2 to 67.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 32804 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
RA wraps around 0/360 boundary: field RA 340.7955 through 0 to 18.4239, gap 18.4239 to 340.7955
Reading UCAC5 zone files...
Searching UCAC5 zones 731 to 788 (Dec 56.2 to 67.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 32806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 32806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits N_match=963 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.290 sigma_q4_arcsec=1.021 n_q1=368 n_q2=156 n_q3=428 n_q4=11 worst_quadrant_to_overall_ratio=3.092
The image catalog is written to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits -region wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits.cat.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_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-10_20.00sec_-4.90C_LIGHTs_0162.fits'
Saving fully-calibrated image wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-15_CI_Cas-02-Q1b1x1_044932_TTUQ1b1x1_628844_ZgVHIEPG/wcs_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163.fits'
Preparing the HTML report for the field Cas-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits at 23:56:18.38 +58:01:21.9: 13.84 +/- 0.05 detection
Forced photometry on wcs_Cas-02-Q1b1x1_2026-01-20_19-34-13_20.00sec_-14.90C_LIGHT_0015.fits at 00:01:19.82 +57:20:32.8: 14.23 +/- 0.07 detection
Forced photometry on wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits at 00:01:19.82 +57:20:32.8: 14.39 +/- 0.09 detection
Forced photometry on wcs_Cas-02-Q1b1x1_2026-02-10_20-23-50_20.00sec_-15.00C_LIGHT_0009.fits at 23:56:18.38 +58:01:21.9: 14.07 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.29 +/- 0.06
Forced photometry reference-image weighted average: 13.90 +/- 0.04
Forced photometry filter KEPT candidate at 23:56:18.38 +58:01:21.9: ref_mag=13.90 +/- 0.04 new_mean_mag=12.6531 delta=1.25 (need > 0.90)
Forced photometry filter KEPT candidate at 00:01:19.82 +57:20:32.8: ref_mag=14.29 +/- 0.06 new_mean_mag=13.2889 delta=1.00 (need > 0.90)
Adding exclusion_list_local.txt__out165419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178247.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 233236_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 233236_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
Rejecting candidate due to large distance (25.3") between the two second-epoch detections
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Considering the candidate 233243_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 233243_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 235482_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 235482_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
**** FOUND 23:06:27.34 +56:43:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239025_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 239025_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
Rejecting candidate due to large distance (46.3") between the two second-epoch detections
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Considering the candidate 243700_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 243700_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
Rejecting candidate due to large distance (49.5") between the two second-epoch detections
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Considering the candidate 245254_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 245254_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
Rejecting candidate due to large distance (88.3") between the two second-epoch detections
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Considering the candidate 246681_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 246681_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 168560_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 168560_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
**** FOUND 23:51:32.41 +57:37:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209339_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 209339_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
**** FOUND 00:00:04.03 +57:06:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 223305_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 223305_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks
**** FOUND 23:49:54.99 +57:35:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93000_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163
The candidate 93000_fd_Cas-02-Q1b1x1_2026-05-15_04-48-53_20.00sec_-4.90C_LIGHTs_0163 did not pass the final checks