This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 16.3553 2461268.8553 12.47 23:49:03.29 -06:40:08.8
84.19475 -64.73940 galactic Aqr Second-epoch detections are separated by 0.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.113 Amalthea 0 -0 0 12.3 0 -0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:49:03.29 -06:40:08.8: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:49:03.29 -06:40:08.8: 15.43 +/- 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,2461268.8553,12.47,0.05,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 20260816.3553 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 16.3553 2461268.8553 12.38 00:09:13.05 -11:04:37.6
89.17021 -71.12676 galactic Cet Second-epoch detections are separated by 0.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.118 Peitho -1 -0 1 12.6 0 -0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:09:13.05 -11:04:37.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:09:13.05 -11:04:37.6: 15.50 +/- 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 08 16.3553* 00 09 13.05 -11 04 37.6 12.4 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,2461268.8553,12.38,0.05,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 20260816.3553 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 16.3553 2461268.8553 13.05 23:43:24.76 -09:40:19.5
77.12598 -66.28865 galactic Aqr Second-epoch detections are separated by 0.6" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.530 Turandot -0 -0 0 13.1 -0 -0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:43:24.76 -09:40:19.5: 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 23:43:24.76 -09:40:19.5: 15.46 +/- 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,2461268.8553,13.05,0.05,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 20260816.3553 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 16.3553 2461268.8553 13.51 23:32:41.18 -07:30:22.9
75.74003 -62.91700 galactic Aqr Second-epoch detections are separated by 1.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.442 Eichsfeldia 0 -0 0 13.4 -0 -0
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:32:41.18 -07:30:22.9: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:32:41.18 -07:30:22.9: 15.29 +/- 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,2461268.8553,13.51,0.05,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 20260816.3553 13.51CV 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: 2461268.85554686 16.08.2026 08:31:49.249 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.91
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 3470
Objects passed selection criteria: 3470
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: 3335.5
Average stars matched: 3269.75 (98.0288 %)
Memory usage VmPeak: 230636 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 16 03:46:59 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: 2461268.85554686 16.08.2026 08:31:49.249 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 91
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 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): 19421
Objects passed selection criteria: 19364
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 18598
Average stars matched: 17515 (94.1768 %)
Memory usage VmPeak: 244444 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 16 03:47:35 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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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: 2461268.85507262
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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits exists and is non-empty
wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits (1st new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Image size: 937.1'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: 23:59:38.209 -09:58:16.16 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 23:59:38.209 -09:58:16.16
Angular distance between the image centers 0.0962 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits (2nd new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
Image size: 937.1'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: 23:59:40.090 -09:58:07.80 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 23:59:40.090 -09:58:07.80
Angular distance between the image centers 0.0898 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 23:59:38.209 -09:58:16.16
Second-epoch second image center 23:59:40.090 -09:58:07.80
Angular distance between the image centers 0.00806 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.DJexJLA5OP
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.IY7jl7DXZN
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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits &> /tmp/tmp.Px5Tf0UpL1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits &> /tmp/tmp.uvnmf2QDbl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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.: -7.91
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.68
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 0 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
2.2 pix fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
2.2 pix fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
Limiting magnitude estimates:
14.7 mag. Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits
14.8 mag. Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits
14.7 mag. fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
14.7 mag. fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.7 (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.DJexJLA5OP (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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/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
############ /tmp/tmp.IY7jl7DXZN (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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/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
############ /tmp/tmp.Px5Tf0UpL1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.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=267, bad_region=864, passed=4117
Got 4117 stars (including 3039 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat
util/solve_plate_with_UCAC5 got 4117 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 351.8781 through 0 to 8.0002, gap 8.0002 to 351.8781
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 -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 2962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2961 matched stars entering correct_measured_positions(), 2961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2961 matched stars entering correct_measured_positions(), 3413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8781 through 0 to 8.0005, gap 8.0005 to 351.8781
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 -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 2962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2960 matched stars entering correct_measured_positions(), 3413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 2960 matched stars entering correct_measured_positions(), 3413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 2960 stars left (next iteration limit 3257)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2960 robust_rms=6.711 arcsec worst_quadrant_rms=11.156 arcsec
SIP_REFIT: SIP order 3 trial: matched=2960 robust_rms=0.458 arcsec worst_quadrant_rms=0.601 arcsec
SIP_REFIT: SIP order 5 trial: matched=2960 robust_rms=0.329 arcsec worst_quadrant_rms=0.378 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2960 robust_rms_before=1.047 arcsec robust_rms_before_corrected=0.317 arcsec robust_rms_after=0.329 arcsec worst_quadrant_rms_before=0.351 worst_quadrant_rms_after=0.378
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.351 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits N_match=2960 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.298 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.380 sigma_q4_arcsec=0.290 n_q1=966 n_q2=552 n_q3=976 n_q4=466 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits -region wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.uvnmf2QDbl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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=274, bad_region=865, passed=4088
Got 4088 stars (including 3005 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat
util/solve_plate_with_UCAC5 got 4088 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 351.8781 through 0 to 8.0031, gap 8.0031 to 351.8781
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 -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 2927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2926 matched stars entering correct_measured_positions(), 2926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2926 matched stars entering correct_measured_positions(), 3381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 351.8782 through 0 to 8.0033, gap 8.0033 to 351.8782
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 -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 2928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2926 matched stars entering correct_measured_positions(), 3381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 2926 matched stars entering correct_measured_positions(), 3381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 2926 stars left (next iteration limit 3218)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2926 robust_rms=6.520 arcsec worst_quadrant_rms=11.776 arcsec
SIP_REFIT: SIP order 3 trial: matched=2926 robust_rms=0.479 arcsec worst_quadrant_rms=0.647 arcsec
SIP_REFIT: SIP order 5 trial: matched=2926 robust_rms=0.344 arcsec worst_quadrant_rms=0.387 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2926 robust_rms_before=1.056 arcsec robust_rms_before_corrected=0.344 arcsec robust_rms_after=0.344 arcsec worst_quadrant_rms_before=0.377 worst_quadrant_rms_after=0.387
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.377 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits N_match=2926 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.289 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.415 sigma_q4_arcsec=0.342 n_q1=935 n_q2=552 n_q3=993 n_q4=446 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits -region wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits to local_wcs_cache/
'wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits' -> 'local_wcs_cache/wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits'
Saving the final (post-refit) wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits to local_wcs_cache/
'wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits' -> 'local_wcs_cache/wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits sigma_overall=0.333 worst_q_ratio=1.142
new2=fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits sigma_overall=0.350 worst_q_ratio=1.185
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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404_astrometric_residuals.png (2960 matched stars from wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405_astrometric_residuals.png (2926 matched stars from wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits'
Saving fully-calibrated image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits'
Preparing the HTML report for the field Cet-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
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 ####
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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits exists and is non-empty
wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits (1st new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Image size: 937.1'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: 23:59:38.209 -09:58:16.16 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 23:59:38.209 -09:58:16.16
Angular distance between the image centers 0.0962 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits (2nd new image)
verification OK: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
Image size: 937.1'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: 23:59:40.090 -09:58:07.80 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 23:59:40.090 -09:58:07.80
Angular distance between the image centers 0.0898 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 23:59:38.209 -09:58:16.16
Second-epoch second image center 23:59:40.090 -09:58:07.80
Angular distance between the image centers 0.00806 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.raeswpupnR
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.9liLzLwNhr
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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits &> /tmp/tmp.DDxnoJF0Y4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits &> /tmp/tmp.85wZvAx6YH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.83
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.83
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 58 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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
2.1 pix fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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
14.9 mag. fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
14.9 mag. fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
All-image limiting magnitude estimate: 14.9 (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.raeswpupnR (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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/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
############ /tmp/tmp.9liLzLwNhr (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_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/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
############ /tmp/tmp.DDxnoJF0Y4 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.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_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.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=9, blended=838, bad_region=3990, passed=23056
Got 23056 stars (including 18402 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat
util/solve_plate_with_UCAC5 got 23056 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 351.8541 through 0 to 8.0002, gap 8.0002 to 351.8541
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 -15.2 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 20003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 351.8541 through 0 to 8.0005, gap 8.0005 to 351.8541
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 -15.2 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: 4837 matched stars entering correct_measured_positions(), 20003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 20003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4837 stars left (next iteration limit 5321)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.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=4837 robust_rms=6.772 arcsec worst_quadrant_rms=10.303 arcsec
SIP_REFIT: SIP order 3 trial: matched=4837 robust_rms=0.461 arcsec worst_quadrant_rms=0.595 arcsec
SIP_REFIT: SIP order 5 trial: matched=4837 robust_rms=0.346 arcsec worst_quadrant_rms=0.388 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4837 robust_rms_before=1.042 arcsec robust_rms_before_corrected=0.335 arcsec robust_rms_after=0.346 arcsec worst_quadrant_rms_before=0.368 worst_quadrant_rms_after=0.388
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.368 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits N_match=4837 sigma_overall_arcsec=0.348 sigma_q1_arcsec=0.319 sigma_q2_arcsec=0.377 sigma_q3_arcsec=0.384 sigma_q4_arcsec=0.300 n_q1=1560 n_q2=866 n_q3=1569 n_q4=842 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits -region wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.85wZvAx6YH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
WCS_IMAGE_NAME=wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
WCS-calibrated image found: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
Checking if the catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat corresponding to the image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
WCS catalog name: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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=18, blended=804, bad_region=4050, passed=23197
Got 23197 stars (including 18524 good ones) from the SExtractor catalog wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat
util/solve_plate_with_UCAC5 got 23197 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 351.8609 through 0 to 8.0031, gap 8.0031 to 351.8609
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 -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4845 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4838 matched stars entering correct_measured_positions(), 20103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8610 through 0 to 8.0033, gap 8.0033 to 351.8610
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 -15.2 to -4.7)
Done reading UCAC5 zone files...
Matched 4845 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 20103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4837 matched stars entering correct_measured_positions(), 20103 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4837 stars left (next iteration limit 5321)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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=4837 robust_rms=6.788 arcsec worst_quadrant_rms=10.283 arcsec
SIP_REFIT: SIP order 3 trial: matched=4837 robust_rms=0.491 arcsec worst_quadrant_rms=0.647 arcsec
SIP_REFIT: SIP order 5 trial: matched=4837 robust_rms=0.371 arcsec worst_quadrant_rms=0.423 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4837 robust_rms_before=1.051 arcsec robust_rms_before_corrected=0.361 arcsec robust_rms_after=0.371 arcsec worst_quadrant_rms_before=0.394 worst_quadrant_rms_after=0.423
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.394 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits N_match=4837 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.311 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.342 n_q1=1554 n_q2=869 n_q3=1573 n_q4=841 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits -region wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-08_20.00sec_-0.00C_LIGHT_0404.fits
Saving fully-calibrated image wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Cet-05-Q2b1x1_034439_TTUQ2b1x1_2670953_QJpJf1lG/wcs_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405.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 23:35:29.23 -07:57:25.6: 13.46 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:44:33.12 -11:37:14.1: 13.27 +/- 0.05 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:55:27.97 -08:53:58.2: 13.95 +/- 0.08 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:56:09.51 -08:03:53.0: 13.75 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:33:41.40 -06:46:10.2: 14.01 +/- 0.12 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:08:45.27 -06:28:02.1: 13.36 +/- 0.05 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:13:02.69 -05:59:51.0: 13.77 +/- 0.08 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:42:48.69 -12:57:57.5: 13.18 +/- 0.05 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:54:35.19 -07:43:44.3: 12.82 +/- 0.03 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:08:45.27 -06:28:02.1: 13.94 +/- 0.09 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:55:27.97 -08:53:58.2: 14.24 +/- 0.11 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:35:29.23 -07:57:25.6: 13.76 +/- 0.09 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:42:48.69 -12:57:57.5: 13.37 +/- 0.06 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:44:33.12 -11:37:14.1: 13.40 +/- 0.06 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:33:41.40 -06:46:10.2: 13.91 +/- 0.11 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:56:09.51 -08:03:53.0: 13.81 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:13:02.69 -05:59:51.0: 13.92 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.07
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Forced photometry reference-image weighted average: 13.58 +/- 0.05
Forced photometry filter REJECTED candidate at 23:55:27.97 -08:53:58.2: ref_mag=14.06 +/- 0.07 new_mean_mag=14.2761 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:35:29.23 -07:57:25.6: ref_mag=13.58 +/- 0.05 new_mean_mag=14.1788 delta=-0.60 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:08:45.27 -06:28:02.1: ref_mag=13.52 +/- 0.04 new_mean_mag=14.0649 delta=-0.54 (need > 0.90)
Forced photometry reference-image weighted average: 13.95 +/- 0.08
Forced photometry reference-image weighted average: 13.33 +/- 0.04
Forced photometry reference-image weighted average: 13.26 +/- 0.04
Forced photometry reference-image weighted average: 13.78 +/- 0.05
Forced photometry reference-image weighted average: 13.85 +/- 0.06
Forced photometry filter REJECTED candidate at 23:33:41.40 -06:46:10.2: ref_mag=13.95 +/- 0.08 new_mean_mag=14.2371 delta=-0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:44:33.12 -11:37:14.1: ref_mag=13.33 +/- 0.04 new_mean_mag=13.9365 delta=-0.61 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:56:09.51 -08:03:53.0: ref_mag=13.78 +/- 0.05 new_mean_mag=14.1496 delta=-0.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:42:48.69 -12:57:57.5: ref_mag=13.26 +/- 0.04 new_mean_mag=13.7635 delta=-0.50 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:13:02.69 -05:59:51.0: ref_mag=13.85 +/- 0.06 new_mean_mag=14.1636 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:54:35.19 -07:43:44.3: 12.86 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.84 +/- 0.02
Forced photometry filter REJECTED candidate at 23:54:35.19 -07:43:44.3: ref_mag=12.84 +/- 0.02 new_mean_mag=13.2937 delta=-0.46 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:49:03.29 -06:40:08.8: 15.40 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:49:03.29 -06:40:08.8: 15.43 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:48:06.66 -07:36:47.9: 12.81 +/- 0.03 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:09:13.05 -11:04:37.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:32:41.18 -07:30:22.9: 15.21 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:59:45.78 -05:52:35.0: 12.55 +/- 0.03 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:43:24.76 -09:40:19.5: 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 23:52:48.96 -06:31:08.4: 13.24 +/- 0.05 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:48:06.66 -07:36:47.9: 13.03 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.03
Forced photometry filter REJECTED candidate at 23:48:06.66 -07:36:47.9: ref_mag=12.90 +/- 0.03 new_mean_mag=13.2595 delta=-0.36 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:32:41.18 -07:30:22.9: 15.29 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:09:13.05 -11:04:37.6: 15.50 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:43:24.76 -09:40:19.5: 15.46 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:59:45.78 -05:52:35.0: 12.52 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.02
Forced photometry filter REJECTED candidate at 23:59:45.78 -05:52:35.0: ref_mag=12.53 +/- 0.02 new_mean_mag=12.5853 delta=-0.05 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:52:48.96 -06:31:08.4: 13.23 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.03
Forced photometry filter REJECTED candidate at 23:52:48.96 -06:31:08.4: ref_mag=13.24 +/- 0.03 new_mean_mag=13.5372 delta=-0.30 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:10:12.61 -12:23:47.7: 13.60 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:59:51.08 -13:24:00.7: 13.77 +/- 0.08 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:56:18.85 -09:31:11.5: 13.85 +/- 0.09 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:34:13.47 -06:06:14.5: 14.48 +/- 0.19 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:00:47.30 -09:01:10.5: 13.66 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:10:12.61 -12:23:47.7: 13.73 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.05
Forced photometry filter REJECTED candidate at 00:10:12.61 -12:23:47.7: ref_mag=13.66 +/- 0.05 new_mean_mag=13.9238 delta=-0.26 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:56:18.85 -09:31:11.5: 13.80 +/- 0.08 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:59:51.08 -13:24:00.7: 13.87 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.06
Forced photometry reference-image weighted average: 13.82 +/- 0.06
Forced photometry filter REJECTED candidate at 23:56:18.85 -09:31:11.5: ref_mag=13.82 +/- 0.06 new_mean_mag=14.0925 delta=-0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:59:51.08 -13:24:00.7: ref_mag=13.82 +/- 0.06 new_mean_mag=13.9976 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:34:13.47 -06:06:14.5: 14.63 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.55 +/- 0.14
Forced photometry filter REJECTED candidate at 23:34:13.47 -06:06:14.5: ref_mag=14.55 +/- 0.14 new_mean_mag=14.3493 delta=0.20 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:00:47.30 -09:01:10.5: 13.85 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.74 +/- 0.05
Forced photometry filter REJECTED candidate at 00:00:47.30 -09:01:10.5: ref_mag=13.74 +/- 0.05 new_mean_mag=14.1268 delta=-0.38 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:52:43.34 -06:40:27.7: 14.34 +/- 0.13 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 00:03:22.00 -10:46:16.7: 13.75 +/- 0.07 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:34:38.18 -07:08:38.1: 14.47 +/- 0.18 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:37:54.84 -10:48:25.6: 14.35 +/- 0.15 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:32:59.78 -08:43:16.0: 14.52 +/- 0.19 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:33:25.40 -09:29:11.6: 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 23:52:43.34 -06:40:27.7: 14.22 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.27 +/- 0.09
Forced photometry filter REJECTED candidate at 23:52:43.34 -06:40:27.7: ref_mag=14.27 +/- 0.09 new_mean_mag=14.2892 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:34:38.18 -07:08:38.1: 14.66 +/- 0.20 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 00:03:22.00 -10:46:16.7: 13.91 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.56 +/- 0.14
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:37:54.84 -10:48:25.6: 14.37 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.82 +/- 0.05
Forced photometry filter REJECTED candidate at 23:34:38.18 -07:08:38.1: ref_mag=14.56 +/- 0.14 new_mean_mag=14.4402 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:03:22.00 -10:46:16.7: ref_mag=13.82 +/- 0.05 new_mean_mag=14.0988 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 14.36 +/- 0.11
Forced photometry filter REJECTED candidate at 23:37:54.84 -10:48:25.6: ref_mag=14.36 +/- 0.11 new_mean_mag=14.2985 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:32:59.78 -08:43:16.0: 14.67 +/- 0.21 detection
Forced photometry reference-image weighted average: 14.59 +/- 0.14
Forced photometry filter REJECTED candidate at 23:32:59.78 -08:43:16.0: ref_mag=14.59 +/- 0.14 new_mean_mag=14.4302 delta=0.16 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:33:25.40 -09:29:11.6: 14.38 +/- 0.16 detection
Forced photometry reference-image weighted average: 14.36 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:25.40 -09:29:11.6: ref_mag=14.36 +/- 0.11 new_mean_mag=14.3577 delta=0.01 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:33:35.61 -10:30:37.7: 14.45 +/- 0.18 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:33:33.74 -09:44:19.7: 14.21 +/- 0.14 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:43:59.39 -08:18:31.8: 14.53 +/- 0.17 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:54:09.84 -09:18:47.6: 14.38 +/- 0.15 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:33:35.61 -10:30:37.7: 14.22 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.30 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:35.61 -10:30:37.7: ref_mag=14.30 +/- 0.11 new_mean_mag=14.2581 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-21_05-32-04_20.00sec_5.00C_LIGHT_1021.fits at 23:37:01.70 -12:30:30.8: 14.81 +/- 0.25 detection
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:33:33.74 -09:44:19.7: 14.55 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.11
Forced photometry filter REJECTED candidate at 23:33:33.74 -09:44:19.7: ref_mag=14.34 +/- 0.11 new_mean_mag=14.3070 delta=0.03 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:43:59.39 -08:18:31.8: 14.39 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.45 +/- 0.11
Forced photometry filter REJECTED candidate at 23:43:59.39 -08:18:31.8: ref_mag=14.45 +/- 0.11 new_mean_mag=14.2739 delta=0.18 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:54:09.84 -09:18:47.6: 14.30 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.34 +/- 0.10
Forced photometry filter REJECTED candidate at 23:54:09.84 -09:18:47.6: ref_mag=14.34 +/- 0.10 new_mean_mag=14.3651 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Cet-05-Q2b1x1_2026-07-22_05-26-37_20.00sec_5.00C_LIGHT_0490.fits at 23:37:01.70 -12:30:30.8: 14.74 +/- 0.22 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.17
Forced photometry filter REJECTED candidate at 23:37:01.70 -12:30:30.8: ref_mag=14.77 +/- 0.17 new_mean_mag=14.4237 delta=0.35 (need > 0.90)
Adding exclusion_list_local.txt__out32180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32260.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 43s
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: 3s
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Considering the candidate 32125_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32125_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32126_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32126_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32128_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32128_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32129_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32129_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32130_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32130_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32131_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32131_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32132_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32132_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32133_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32133_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32136_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32136_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32158_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32158_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.2") between the two second-epoch detections
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Considering the candidate 32176_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32176_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 32180_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
Preparing report for the candidate 32180_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
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Considering the candidate 32186_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
Preparing report for the candidate 32186_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
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Considering the candidate 32194_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32194_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32206_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32206_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 32209_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32209_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 32215_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
Preparing report for the candidate 32215_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
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Considering the candidate 32237_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32237_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32248_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32248_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 32260_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
Preparing report for the candidate 32260_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
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Considering the candidate 32262_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32262_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 32267_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32267_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32268_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32268_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 32270_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32270_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 32279_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32279_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 32281_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32281_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 32284_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32284_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.6") between the two second-epoch detections
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Considering the candidate 32290_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32290_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 32295_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32295_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 32329_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32329_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 32333_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32333_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.3") between the two second-epoch detections
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Considering the candidate 32334_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32334_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.3") between the two second-epoch detections
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Considering the candidate 32336_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32336_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32337_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32337_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 32342_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32342_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32343_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32343_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32351_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32351_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.2") between the two second-epoch detections
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Considering the candidate 32353_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32353_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32355_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32355_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32356_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32356_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 32357_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32357_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.9") between the two second-epoch detections
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Considering the candidate 32358_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32358_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (30.0") between the two second-epoch detections
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Considering the candidate 32361_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32361_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.7") between the two second-epoch detections
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Considering the candidate 32367_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32367_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32372_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32372_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 32379_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32379_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32385_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32385_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32386_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32386_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32387_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32387_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32390_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32390_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32397_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32397_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32398_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32398_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32414_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32414_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32427_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32427_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 32437_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32437_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32445_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32445_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
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Considering the candidate 32468_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32468_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks
Rejecting candidate due to large distance (28.8") between the two second-epoch detections
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Considering the candidate 32496_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405
The candidate 32496_fd_Cet-05-Q2b1x1_2026-08-16_03-31-49_20.00sec_-0.00C_LIGHT_0405 did not pass the final checks