This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF
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 09 14.2558 2461297.7558 11.31 23:59:48.24 -07:13:52.6
88.95910 -66.63446 galactic Cet Second-epoch detections are separated by 0.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.106 Dione -0 0 0 11.5 0 0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:59:48.24 -07:13:52.6: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:59:48.24 -07:13:52.6: 15.45 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 14.2558* 23 59 48.24 -07 13 52.6 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461297.7558,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260914.2558 11.31CV 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 09 14.2558 2461297.7558 11.82 23:48:03.86 -13:27:41.0
72.50399 -69.85191 galactic Aqr Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.118 Peitho -0 -0 0 11.9 0 -0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:48:03.86 -13:27:41.0: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:48:03.86 -13:27:41.0: 15.26 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461297.7558,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260914.2558 11.82CV 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 09 14.2558 2461297.7558 13.64 00:11:08.70 -10:47:21.0
90.88085 -71.10913 galactic Cet Second-epoch detections are separated by 1.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1133 Lugduna -0 -0 1 13.5 -0 -0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:11:08.70 -10:47:21.0: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:11:08.70 -10:47:21.0: 15.47 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 14.2558* 00 11 08.70 -10 47 21.0 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461297.7558,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260914.2558 13.64CV 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 09 14.2558 2461297.7558 14.13 23:33:16.80 -05:58:04.2
78.12243 -61.83572 galactic Aqr Second-epoch detections are separated by 1.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.981 Martina -2 1 2 14.1 0 0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:33:16.80 -05:58:04.2: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:33:16.80 -05:58:04.2: 15.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461297.7558,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260914.2558 14.13CV 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: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
First image: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Last image: 2461297.75610105 14.09.2026 06:08:37.131 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.80
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 3494
Objects passed selection criteria: 3492
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 3397.5
Average stars matched: 3330.5 (98.028 %)
Memory usage VmPeak: 230732 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 14 03:32:33 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: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
First image: 2461242.93905227 21.07.2026 10:32:04.116 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Last image: 2461297.75610105 14.09.2026 06:08:37.131 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
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: 9 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 19101
Objects passed selection criteria: 19043
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 18540.8
Average stars matched: 17581.5 (94.8263 %)
Memory usage VmPeak: 245788 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 14 03:35:26 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
SExtractor catalog cache: saved Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.cat to cache
SExtractor catalog cache: saved Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.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/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.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: 2461297.75549763
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_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits exists and is non-empty
wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits exists and is non-empty
wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits exists and is non-empty
wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (1st reference image)
verification OK: wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Image size: 937.6'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:00.437 -10:00:06.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits (1st new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.619 -09:59:45.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 23:59:59.619 -09:59:45.88
Angular distance between the image centers 0.0066 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits (2nd new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.515 -10:00:19.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 00:00:01.515 -10:00:19.39
Angular distance between the image centers 0.0057 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 23:59:59.619 -09:59:45.88
Second-epoch second image center 00:00:01.515 -10:00:19.39
Angular distance between the image centers 0.01213 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits &> /tmp/tmp.87bjm8geE4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits &> /tmp/tmp.yTLDUl3rcm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits &> /tmp/tmp.AAx3LTWxDA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits &> /tmp/tmp.YHho3xH15o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Found non-empty wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
The reference image (wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits) and catalog (wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat) found
'wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 4374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 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 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 deg
Loaded 4197 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): 3165 out of 3236 total matches.
Matched with Tycho-2 3236 out of 4374 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.590100
a=0.000000 b=1.000000 c=22.590100
From vast_summary.log: estimated ref. image limiting mag.: -7.80
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.79
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.79
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 4374 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 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 351.9535 to 8.0780 deg, Dec -15.2625 to -4.6835 deg
Loaded 4197 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): 3165 out of 3236 total matches.
Matched with Tycho-2 3236 out of 4374 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -> calib.txt_param_ref_wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (aperture=7.4)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 4358 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9535 to 8.0779 deg, Dec -15.2626 to -4.6837 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 351.9535 to 8.0779 deg, Dec -15.2626 to -4.6837 deg
Loaded 4197 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): 3202 out of 3251 total matches.
Matched with Tycho-2 3251 out of 4358 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -> calib.txt_param_ref_wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.6 pix Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
2.3 pix Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
2.3 pix fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
2.3 pix fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Limiting magnitude estimates:
14.8 mag. Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
14.9 mag. Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
14.8 mag. fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
14.8 mag. fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.87bjm8geE4 (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits' -> 'wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS-calibrated image found: wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Checking if the catalog wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS catalog name: wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=278, bad_region=897, passed=4374
Got 4374 stars (including 3271 good ones) from the SExtractor catalog wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
util/solve_plate_with_UCAC5 got 4374 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9535 through 0 to 8.0780, gap 8.0780 to 351.9535
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3184 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3182 matched stars entering correct_measured_positions(), 3182 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3182 matched stars entering correct_measured_positions(), 3648 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
RA wraps around 0/360 boundary: field RA 351.9539 through 0 to 8.0778, gap 8.0778 to 351.9539
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3184 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3182 matched stars entering correct_measured_positions(), 3648 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 3182 matched stars entering correct_measured_positions(), 3648 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 3182 stars left (next iteration limit 3500)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits N_match=3182 sigma_overall_arcsec=0.357 sigma_q1_arcsec=0.350 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.389 sigma_q4_arcsec=0.353 n_q1=1080 n_q2=583 n_q3=999 n_q4=520 worst_quadrant_to_overall_ratio=1.090
The image catalog is written to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -region wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.yTLDUl3rcm (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits' -> 'wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS-calibrated image found: wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Checking if the catalog wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS catalog name: wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=264, bad_region=887, passed=4358
Got 4358 stars (including 3264 good ones) from the SExtractor catalog wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
util/solve_plate_with_UCAC5 got 4358 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9535 through 0 to 8.0779, gap 8.0779 to 351.9535
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3179 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3177 matched stars entering correct_measured_positions(), 3177 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3177 matched stars entering correct_measured_positions(), 3631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9539 through 0 to 8.0778, gap 8.0778 to 351.9539
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3179 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3177 matched stars entering correct_measured_positions(), 3631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 3177 matched stars entering correct_measured_positions(), 3631 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 3177 stars left (next iteration limit 3494)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits N_match=3177 sigma_overall_arcsec=0.276 sigma_q1_arcsec=0.274 sigma_q2_arcsec=0.268 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.249 n_q1=1022 n_q2=571 n_q3=1079 n_q4=505 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -region wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.AAx3LTWxDA (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=311, bad_region=866, passed=4228
Got 4228 stars (including 3116 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat
util/solve_plate_with_UCAC5 got 4228 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9542 through 0 to 8.0760, gap 8.0760 to 351.9542
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3033 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3032 matched stars entering correct_measured_positions(), 3032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3032 matched stars entering correct_measured_positions(), 3516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9540 through 0 to 8.0758, gap 8.0758 to 351.9540
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3033 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3031 matched stars entering correct_measured_positions(), 3516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 3031 matched stars entering correct_measured_positions(), 3516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 3031 stars left (next iteration limit 3335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3031 robust_rms=6.326 arcsec worst_quadrant_rms=11.979 arcsec
SIP_REFIT: SIP order 3 trial: matched=3031 robust_rms=0.600 arcsec worst_quadrant_rms=0.777 arcsec
SIP_REFIT: SIP order 5 trial: matched=3031 robust_rms=0.389 arcsec worst_quadrant_rms=0.436 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3031 robust_rms_before=4.512 arcsec robust_rms_before_corrected=0.398 arcsec robust_rms_after=0.389 arcsec worst_quadrant_rms_before=0.436 worst_quadrant_rms_after=0.436
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.436 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits N_match=3031 sigma_overall_arcsec=0.403 sigma_q1_arcsec=0.374 sigma_q2_arcsec=0.449 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.413 n_q1=986 n_q2=547 n_q3=1015 n_q4=483 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits -region wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.YHho3xH15o (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=297, bad_region=864, passed=4214
Got 4214 stars (including 3123 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 4214 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9541 through 0 to 8.0776, gap 8.0776 to 351.9541
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3035 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3034 matched stars entering correct_measured_positions(), 3034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3034 matched stars entering correct_measured_positions(), 3511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 351.9542 through 0 to 8.0779, gap 8.0779 to 351.9542
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 3035 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3033 matched stars entering correct_measured_positions(), 3511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 3033 matched stars entering correct_measured_positions(), 3511 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 3033 stars left (next iteration limit 3337)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3033 robust_rms=6.369 arcsec worst_quadrant_rms=12.681 arcsec
SIP_REFIT: SIP order 3 trial: matched=3033 robust_rms=0.621 arcsec worst_quadrant_rms=0.744 arcsec
SIP_REFIT: SIP order 5 trial: matched=3033 robust_rms=0.390 arcsec worst_quadrant_rms=0.427 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3033 robust_rms_before=1.017 arcsec robust_rms_before_corrected=0.373 arcsec robust_rms_after=0.390 arcsec worst_quadrant_rms_before=0.406 worst_quadrant_rms_after=0.427
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.406 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits N_match=3033 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.433 sigma_q4_arcsec=0.384 n_q1=995 n_q2=545 n_q3=1023 n_q4=470 worst_quadrant_to_overall_ratio=1.119
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits -region wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits to local_wcs_cache/
'wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits' -> 'local_wcs_cache/wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits'
Saving the final (post-refit) wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits to local_wcs_cache/
'wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits' -> 'local_wcs_cache/wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits'
Saving the final (post-refit) wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits to local_wcs_cache/
'wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits' -> 'local_wcs_cache/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits'
Saving the final (post-refit) wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits to local_wcs_cache/
'wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits' -> 'local_wcs_cache/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits sigma_overall=0.357 worst_q_ratio=1.090
ref2=Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits sigma_overall=0.276 worst_q_ratio=1.120
new1=fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits sigma_overall=0.403 worst_q_ratio=1.114
new2=fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits sigma_overall=0.387 worst_q_ratio=1.119
reference average sigma_overall=0.3165 worst_q_ratio=1.105
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021_astrometric_residuals.png (3182 matched stars from wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490_astrometric_residuals.png (3177 matched stars from wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.25 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288_astrometric_residuals.png (3031 matched stars from wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289_astrometric_residuals.png (3033 matched stars from wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits'
Saving fully-calibrated image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits'
Preparing the HTML report for the field Cet-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:32:49.47 -08:01:55.6: 11.88 +/- 0.02 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:59:48.24 -07:13:52.6: 15.39 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:48:03.86 -13:27:41.0: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:32:49.47 -08:01:55.6: 11.89 +/- 0.02 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:59:48.24 -07:13:52.6: 15.45 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:48:03.86 -13:27:41.0: 15.26 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.89 +/- 0.01
Forced photometry filter REJECTED candidate at 23:32:49.47 -08:01:55.6: ref_mag=11.89 +/- 0.01 new_mean_mag=11.8743 delta=0.01 (need > 0.90)
Adding exclusion_list_local.txt__out20190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20191.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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20190_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
Preparing report for the candidate 20190_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20191_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
Preparing report for the candidate 20191_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20192_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 20192_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03145_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 03145_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
**** FOUND 00:13:45.94 -07:48:35.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Cet-05-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 ####
23:59:48.24 -07:13:52.6
23:48:03.86 -13:27:41.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
SExtractor catalog cache: saved Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.cat to cache
SExtractor catalog cache: saved Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Creating symlink local_wcs_cache/wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
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_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits exists and is non-empty
wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits exists and is non-empty
wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits exists and is non-empty
wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (1st reference image)
verification OK: wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Image size: 937.6'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 00:00:00.437 -10:00:06.37 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits (1st new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Image size: 937.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.619 -09:59:45.88 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 23:59:59.619 -09:59:45.88
Angular distance between the image centers 0.0066 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits (2nd new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.515 -10:00:19.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.437 -10:00:06.37
Second-epoch image center 00:00:01.515 -10:00:19.39
Angular distance between the image centers 0.0057 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 23:59:59.619 -09:59:45.88
Second-epoch second image center 00:00:01.515 -10:00:19.39
Angular distance between the image centers 0.01213 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits &> /tmp/tmp.SNo4Cry4dJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits &> /tmp/tmp.h9qXG4Xlpg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits &> /tmp/tmp.iThgqzvZtV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits &> /tmp/tmp.FEYafU2sN7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.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_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Found non-empty wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits and wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
The reference image (wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits) and catalog (wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat) found
'wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 22737 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 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 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 deg
Loaded 4214 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): 3418 out of 3629 total matches.
Matched with Tycho-2 3629 out of 22737 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.414650
a=0.000000 b=1.000000 c=22.414650
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 22737 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 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 351.9459 to 8.0985 deg, Dec -15.2699 to -4.6646 deg
Loaded 4214 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): 3418 out of 3629 total matches.
Matched with Tycho-2 3629 out of 22737 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -> calib.txt_param_ref_wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (aperture=5.5)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 23415 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9462 to 8.0901 deg, Dec -15.2699 to -4.6646 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 351.9462 to 8.0901 deg, Dec -15.2699 to -4.6646 deg
Loaded 4212 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): 3459 out of 3633 total matches.
Matched with Tycho-2 3633 out of 23415 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Forced-photometry filter: calibrated wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -> calib.txt_param_ref_wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
2.2 pix Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
2.1 pix fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
2.1 pix fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Limiting magnitude estimates:
14.9 mag. Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
15.0 mag. Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
15.1 mag. fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
15.1 mag. fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.SNo4Cry4dJ (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits' -> 'wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS-calibrated image found: wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
Checking if the catalog wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
WCS catalog name: wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=913, bad_region=4921, passed=22724
Got 22724 stars (including 17090 good ones) from the SExtractor catalog wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat
util/solve_plate_with_UCAC5 got 22724 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9459 through 0 to 8.0985, gap 8.0985 to 351.9459
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 18888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 351.9463 through 0 to 8.0984, gap 8.0984 to 351.9463
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 18888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4836 matched stars entering correct_measured_positions(), 18888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4836 stars left (next iteration limit 5319)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits N_match=4836 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.327 sigma_q3_arcsec=0.454 sigma_q4_arcsec=0.366 n_q1=1598 n_q2=928 n_q3=1483 n_q4=827 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits -region wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.h9qXG4Xlpg (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits' -> 'wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS_IMAGE_NAME=wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS-calibrated image found: wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
Checking if the catalog wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits alredy exist and is non-empty...
Catalog wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat corresponding to the image wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
WCS catalog name: wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=831, bad_region=4531, passed=23408
Got 23408 stars (including 18214 good ones) from the SExtractor catalog wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat
util/solve_plate_with_UCAC5 got 23408 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9462 through 0 to 8.0901, gap 8.0901 to 351.9462
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 4838 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 19951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9465 through 0 to 8.0901, gap 8.0901 to 351.9465
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4843 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 19951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 19951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4838 stars left (next iteration limit 5321)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits N_match=4838 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.286 sigma_q2_arcsec=0.279 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.293 n_q1=1569 n_q2=893 n_q3=1543 n_q4=833 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits -region wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.iThgqzvZtV (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=849, bad_region=4555, passed=23577
Got 23577 stars (including 18346 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat
util/solve_plate_with_UCAC5 got 23577 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9470 through 0 to 8.0880, gap 8.0880 to 351.9470
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 4831 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4831 matched stars entering correct_measured_positions(), 20083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9468 through 0 to 8.0878, gap 8.0878 to 351.9468
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4837 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 20083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 20083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4829 stars left (next iteration limit 5314)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4829 robust_rms=6.673 arcsec worst_quadrant_rms=10.407 arcsec
SIP_REFIT: SIP order 3 trial: matched=4829 robust_rms=0.598 arcsec worst_quadrant_rms=0.758 arcsec
SIP_REFIT: SIP order 5 trial: matched=4829 robust_rms=0.406 arcsec worst_quadrant_rms=0.454 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4829 robust_rms_before=4.378 arcsec robust_rms_before_corrected=0.404 arcsec robust_rms_after=0.406 arcsec worst_quadrant_rms_before=0.439 worst_quadrant_rms_after=0.454
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.439 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits N_match=4829 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.371 sigma_q2_arcsec=0.431 sigma_q3_arcsec=0.455 sigma_q4_arcsec=0.371 n_q1=1579 n_q2=894 n_q3=1518 n_q4=838 worst_quadrant_to_overall_ratio=1.123
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits -region wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.FEYafU2sN7 (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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=844, bad_region=4540, passed=23513
Got 23513 stars (including 18301 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 23513 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9466 through 0 to 8.0969, gap 8.0969 to 351.9466
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 4832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 20027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 351.9467 through 0 to 8.0973, gap 8.0973 to 351.9467
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 428 (Dec -15.3 to -4.7)
Done reading UCAC5 zone files...
Matched 4837 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 20027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4830 matched stars entering correct_measured_positions(), 20027 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4830 stars left (next iteration limit 5315)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4830 robust_rms=6.710 arcsec worst_quadrant_rms=10.264 arcsec
SIP_REFIT: SIP order 3 trial: matched=4830 robust_rms=0.588 arcsec worst_quadrant_rms=0.743 arcsec
SIP_REFIT: SIP order 5 trial: matched=4830 robust_rms=0.408 arcsec worst_quadrant_rms=0.467 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4830 robust_rms_before=1.003 arcsec robust_rms_before_corrected=0.394 arcsec robust_rms_after=0.408 arcsec worst_quadrant_rms_before=0.436 worst_quadrant_rms_after=0.467
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.436 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits N_match=4830 sigma_overall_arcsec=0.411 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.430 sigma_q3_arcsec=0.453 sigma_q4_arcsec=0.420 n_q1=1593 n_q2=896 n_q3=1509 n_q4=832 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits -region wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-07-44_20.00sec_-0.00C_LIGHT_0288.fits
Saving fully-calibrated image wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.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_2026-09-14_CI_Cet-05-Q2b1x1_015057_TTUQ2b1x1_3093600_eeAYhuhF/wcs_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289.fits
Preparing the HTML report for the field Cet-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:33:41.36 -06:46:14.2: 13.97 +/- 0.12 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:56:09.60 -08:03:52.9: 13.82 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:33:16.80 -05:58:04.2: 15.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:10:53.94 -12:53:49.0: 12.33 +/- 0.02 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:37:57.96 -14:09:53.4: 14.23 +/- 0.15 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:03:22.12 -10:46:14.2: 13.82 +/- 0.08 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:17:43.36 -11:13:12.0: 11.60 +/- 0.01 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:11:08.70 -10:47:21.0: 15.44 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:32:27.42 -10:44:46.8: 14.43 +/- 0.18 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:37:54.88 -10:48:26.2: 14.36 +/- 0.15 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:11:08.70 -10:47:21.0: 15.47 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:33:16.80 -05:58:04.2: 15.23 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:17:43.36 -11:13:12.0: 11.80 +/- 0.01 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:56:09.60 -08:03:52.9: 13.83 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:37:57.96 -14:09:53.4: 14.35 +/- 0.16 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:33:41.36 -06:46:14.2: 13.81 +/- 0.10 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:10:53.94 -12:53:49.0: 12.65 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.83 +/- 0.05
Forced photometry reference-image weighted average: 14.28 +/- 0.11
Forced photometry reference-image weighted average: 11.68 +/- 0.01
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:03:22.12 -10:46:14.2: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.07
Forced photometry filter REJECTED candidate at 23:56:09.60 -08:03:52.9: ref_mag=13.83 +/- 0.05 new_mean_mag=14.1198 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:37:57.96 -14:09:53.4: ref_mag=14.28 +/- 0.11 new_mean_mag=14.0801 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 12.45 +/- 0.02
Forced photometry filter REJECTED candidate at 00:17:43.36 -11:13:12.0: ref_mag=11.68 +/- 0.01 new_mean_mag=11.9290 delta=-0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:33:41.36 -06:46:14.2: ref_mag=13.87 +/- 0.07 new_mean_mag=14.0370 delta=-0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:10:53.94 -12:53:49.0: ref_mag=12.45 +/- 0.02 new_mean_mag=13.0038 delta=-0.55 (need > 0.90)
Forced photometry reference-image weighted average: 13.86 +/- 0.06
Forced photometry filter REJECTED candidate at 00:03:22.12 -10:46:14.2: ref_mag=13.86 +/- 0.06 new_mean_mag=13.9876 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:32:27.42 -10:44:46.8: 14.30 +/- 0.15 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:37:54.88 -10:48:26.2: 14.38 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.12
Forced photometry filter REJECTED candidate at 23:32:27.42 -10:44:46.8: ref_mag=14.36 +/- 0.12 new_mean_mag=14.2248 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 14.37 +/- 0.11
Forced photometry filter REJECTED candidate at 23:37:54.88 -10:48:26.2: ref_mag=14.37 +/- 0.11 new_mean_mag=14.2707 delta=0.10 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:35:53.85 -10:28:23.3: 14.48 +/- 0.17 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:48:48.81 -13:17:41.6: 14.52 +/- 0.16 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:52:43.41 -06:40:26.2: 14.27 +/- 0.13 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:43:04.12 -12:51:52.0: 14.39 +/- 0.15 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:35:53.85 -10:28:23.3: 14.49 +/- 0.17 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:52:43.41 -06:40:26.2: 14.18 +/- 0.11 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:43:04.12 -12:51:52.0: 14.50 +/- 0.17 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:48:48.81 -13:17:41.6: 14.89 +/- 0.23 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.12
Forced photometry reference-image weighted average: 14.22 +/- 0.08
Forced photometry reference-image weighted average: 14.44 +/- 0.11
Forced photometry filter REJECTED candidate at 23:35:53.85 -10:28:23.3: ref_mag=14.48 +/- 0.12 new_mean_mag=14.3530 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:52:43.41 -06:40:26.2: ref_mag=14.22 +/- 0.08 new_mean_mag=14.2467 delta=-0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:43:04.12 -12:51:52.0: ref_mag=14.44 +/- 0.11 new_mean_mag=14.4189 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 14.65 +/- 0.13
Forced photometry filter REJECTED candidate at 23:48:48.81 -13:17:41.6: ref_mag=14.65 +/- 0.13 new_mean_mag=14.4004 delta=0.25 (need > 0.90)
Adding exclusion_list_local.txt__out32161.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32176.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 32126_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32126_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32129_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32129_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32133_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32133_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
**** FOUND 23:59:48.23 -07:13:52.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32137_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32137_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
**** FOUND 23:48:03.85 -13:27:41.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32140_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32140_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32161_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
Preparing report for the candidate 32161_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
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Considering the candidate 32169_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32169_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32175_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32175_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32176_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
Preparing report for the candidate 32176_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
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Considering the candidate 32182_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32182_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32186_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32186_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32196_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32196_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32199_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32199_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32201_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32201_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32215_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32215_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 32216_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 32216_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks
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Considering the candidate 21120_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289
The candidate 21120_fd_Cet-05-Q2b1x1_2026-09-14_01-08-37_20.00sec_-0.00C_LIGHT_0289 did not pass the final checks