This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e
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 10 09.3796 2461322.8796 13.02 08:57:02.66 +20:16:30.7
206.83331 36.36971 galactic Cnc Second-epoch detections are separated by 1.1" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.521 Brixia 0 -0 0 13.4 -0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:57:02.66 +20:16:30.7: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:57:02.66 +20:16:30.7: 16.15 +/- 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,2461322.8796,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3796 13.02CV 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 10 09.3796 2461322.8796 12.73 09:38:42.43 +21:19:11.8
209.60542 45.93745 galactic Leo Second-epoch detections are separated by 1.4" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.68 Leto 1 -0 1 13.0 0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:38:42.43 +21:19:11.8: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:38:42.43 +21:19:11.8: 16.04 +/- 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 10 09.3796* 09 38 42.43 +21 19 11.8 12.7 U Leo 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,2461322.8796,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3796 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 09.3796 2461322.8796 12.97 09:13:56.00 +22:37:57.3
205.53917 40.83899 galactic Cnc Second-epoch detections are separated by 1.5" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.145 Adeona -0 -0 0 13.3 0 -0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:13:56.00 +22:37:57.3: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:13:56.00 +22:37:57.3: 16.27 +/- 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,2461322.8796,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3796 12.97CV 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 10 09.3796 2461322.8796 13.59 09:43:15.25 +22:04:28.7
209.00705 47.16864 galactic Leo Second-epoch detections are separated by 1.1" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.87 Sylvia 1 1 1 13.7 0 -0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:43:15.25 +22:04:28.7: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:43:15.25 +22:04:28.7: 16.01 +/- 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 10 09.3796* 09 43 15.25 +22 04 28.7 13.6 U Leo 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,2461322.8796,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3796 13.59CV 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 10 09.3796 2461322.8796 14.35 09:03:29.69 +20:19:28.0
207.40044 37.81378 galactic Cnc Second-epoch detections are separated by 3.3" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.410 Chloris -0 1 1 14.6 0 0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:03:29.69 +20:19:28.0: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:03:29.69 +20:19:28.0: 16.23 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461322.8796,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261009.3796 14.35CV 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: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461322.87998296 09.10.2026 09:07:00.528 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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): 8793
Objects passed selection criteria: 8769
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 7008.75
Average stars matched: 6798.25 (96.9966 %)
Memory usage VmPeak: 241300 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 04:11:30 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: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461322.87998296 09.10.2026 09:07:00.528 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 36
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.04
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: 14 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): 47870
Objects passed selection criteria: 47740
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 39564.8
Average stars matched: 38139.8 (96.3983 %)
Memory usage VmPeak: 269060 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Oct 9 04:12:21 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461322.87925252
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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:50.704 +21:59:59.79 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Image size: 945.5'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:45.909 +22:00:44.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:45.909 +22:00:44.31
Angular distance between the image centers 0.0223 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Image size: 945.3'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:43.378 +22:00:14.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:43.378 +22:00:14.55
Angular distance between the image centers 0.0286 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 09:13:45.909 +22:00:44.31
Second-epoch second image center 09:13:43.378 +22:00:14.55
Angular distance between the image centers 0.01280 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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.22OQfZvKAl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.l0kjLwejbt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits &> /tmp/tmp.70R1EMHTX6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.jiBn9n4jjI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat' -> 'wcsmag.cat'
Read 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0580 deg, Dec +16.3325 to +27.3464 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 129.4936 to 147.0580 deg, Dec 16.3325 to 27.3464 deg
Loaded 6006 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): 4510 out of 4801 total matches.
Matched with Tycho-2 4801 out of 9058 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.920200
a=0.000000 b=1.000000 c=22.920200
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0580 deg, Dec +16.3325 to +27.3464 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 129.4936 to 147.0580 deg, Dec 16.3325 to 27.3464 deg
Loaded 6006 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): 4510 out of 4801 total matches.
Matched with Tycho-2 4801 out of 9058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=6.3)
Read 9037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0623 deg, Dec +16.3327 to +27.3523 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 129.4936 to 147.0623 deg, Dec 16.3327 to 27.3523 deg
Loaded 6008 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): 4486 out of 4794 total matches.
Matched with Tycho-2 4794 out of 9037 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=6.3)
____ 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:
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
15.6 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.6 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
14.6 mag. fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
14.7 mag. fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.6 (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.22OQfZvKAl (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=691, bad_region=0, passed=9058
Got 9058 stars (including 8360 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 9058 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 4821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 4811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 9058 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
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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 4821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 9058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 9058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4812 stars left (next iteration limit 5292)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=4812 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.464 sigma_q2_arcsec=0.334 sigma_q3_arcsec=0.356 sigma_q4_arcsec=0.329 n_q1=1361 n_q2=1105 n_q3=1319 n_q4=1027 worst_quadrant_to_overall_ratio=1.245
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.l0kjLwejbt (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=724, bad_region=0, passed=9037
Got 9037 stars (including 8310 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 9037 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 4814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 9037 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
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 9037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 9037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4814 stars left (next iteration limit 5295)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=4814 sigma_overall_arcsec=0.398 sigma_q1_arcsec=0.486 sigma_q2_arcsec=0.381 sigma_q3_arcsec=0.372 sigma_q4_arcsec=0.362 n_q1=1349 n_q2=1112 n_q3=1325 n_q4=1028 worst_quadrant_to_overall_ratio=1.221
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.70R1EMHTX6 (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=331, bad_region=0, passed=5013
Got 5013 stars (including 4675 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 5013 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.5'
Seting catalog search parameters based on the expected field of view 945.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013132 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010506 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 4514 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4504 matched stars entering correct_measured_positions(), 4504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4504 matched stars entering correct_measured_positions(), 5013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 4513 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4504 matched stars entering correct_measured_positions(), 5013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4504 matched stars entering correct_measured_positions(), 5013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4504 stars left (next iteration limit 4954)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4504 robust_rms=10.612 arcsec worst_region_rms=17.441 arcsec outer_annulus_rms=17.441 arcsec
SIP_REFIT: SIP order 3 trial: matched=4504 robust_rms=0.802 arcsec worst_region_rms=1.076 arcsec outer_annulus_rms=0.872 arcsec
SIP_REFIT: SIP order 5 trial: matched=4504 robust_rms=0.507 arcsec worst_region_rms=0.625 arcsec outer_annulus_rms=0.450 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4504 robust_rms_before=1.693 arcsec robust_rms_before_corrected=0.457 arcsec robust_rms_after=0.507 arcsec worst_region_rms_before=0.585 worst_region_rms_after=0.625 outer_annulus_rms_before=1.814 outer_annulus_rms_after=0.450
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.585 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits worst_region_rms_kept=0.585 arcsec robust_rms_kept=0.457 arcsec matched=4504
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits N_match=4504 sigma_overall_arcsec=0.463 sigma_q1_arcsec=0.432 sigma_q2_arcsec=0.571 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.520 n_q1=1405 n_q2=869 n_q3=1373 n_q4=857 worst_quadrant_to_overall_ratio=1.234
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.jiBn9n4jjI (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=380, bad_region=0, passed=5116
Got 5116 stars (including 4723 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 5116 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.3'
Seting catalog search parameters based on the expected field of view 945.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013129 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010503 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 4554 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4546 matched stars entering correct_measured_positions(), 4546 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4546 matched stars entering correct_measured_positions(), 5116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 4555 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4546 matched stars entering correct_measured_positions(), 5116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 4546 matched stars entering correct_measured_positions(), 5116 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4546 stars left (next iteration limit 5000)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4546 robust_rms=10.874 arcsec worst_region_rms=18.122 arcsec outer_annulus_rms=18.122 arcsec
SIP_REFIT: SIP order 3 trial: matched=4546 robust_rms=0.789 arcsec worst_region_rms=1.170 arcsec outer_annulus_rms=0.872 arcsec
SIP_REFIT: SIP order 5 trial: matched=4546 robust_rms=0.495 arcsec worst_region_rms=0.634 arcsec outer_annulus_rms=0.425 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4546 robust_rms_before=1.605 arcsec robust_rms_before_corrected=0.445 arcsec robust_rms_after=0.495 arcsec worst_region_rms_before=0.561 worst_region_rms_after=0.634 outer_annulus_rms_before=1.698 outer_annulus_rms_after=0.425
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.561 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits worst_region_rms_kept=0.561 arcsec robust_rms_kept=0.445 arcsec matched=4546
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits N_match=4546 sigma_overall_arcsec=0.459 sigma_q1_arcsec=0.434 sigma_q2_arcsec=0.556 sigma_q3_arcsec=0.388 sigma_q4_arcsec=0.554 n_q1=1412 n_q2=899 n_q3=1360 n_q4=875 worst_quadrant_to_overall_ratio=1.210
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
Saving the final (post-refit) wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
Saving the final (post-refit) wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits'
Saving the final (post-refit) wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits sigma_overall=0.373 worst_q_ratio=1.245
ref2=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits sigma_overall=0.398 worst_q_ratio=1.221
new1=fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits sigma_overall=0.463 worst_q_ratio=1.234
new2=fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits sigma_overall=0.459 worst_q_ratio=1.210
reference average sigma_overall=0.3855 worst_q_ratio=1.233
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199_astrometric_residuals.png (4812 matched stars from wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200_astrometric_residuals.png (4814 matched stars from wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446_astrometric_residuals.png (4504 matched stars from wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447_astrometric_residuals.png (4546 matched stars from wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits'
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Checking 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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:50.704 +21:59:59.79 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Image size: 945.5'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:45.909 +22:00:44.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:45.909 +22:00:44.31
Angular distance between the image centers 0.0223 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Image size: 945.3'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:43.378 +22:00:14.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.704 +21:59:59.79
Second-epoch image center 09:13:43.378 +22:00:14.55
Angular distance between the image centers 0.0286 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 09:13:45.909 +22:00:44.31
Second-epoch second image center 09:13:43.378 +22:00:14.55
Angular distance between the image centers 0.01280 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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.0d3nZCU6jA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.HCHmg8xxYd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits &> /tmp/tmp.EYQZkU7SDP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits &> /tmp/tmp.fCAanfXxvN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat' -> 'wcsmag.cat'
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0734 deg, Dec +16.3325 to +27.3500 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 129.4936 to 147.0734 deg, Dec 16.3325 to 27.3500 deg
Loaded 6016 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): 4201 out of 4841 total matches.
Matched with Tycho-2 4841 out of 50507 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.814600
a=0.000000 b=1.000000 c=22.814600
From vast_summary.log: estimated ref. image limiting mag.: -7.04
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.77
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.77
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4936 to 147.0734 deg, Dec +16.3325 to +27.3500 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 129.4936 to 147.0734 deg, Dec 16.3325 to 27.3500 deg
Loaded 6016 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): 4201 out of 4841 total matches.
Matched with Tycho-2 4841 out of 50507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=5.0)
Read 50709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4911 to 147.0623 deg, Dec +16.3281 to +27.3564 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 129.4911 to 147.0623 deg, Dec 16.3281 to 27.3564 deg
Loaded 6019 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): 4178 out of 4842 total matches.
Matched with Tycho-2 4842 out of 50709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 36 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
2.3 pix fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Limiting magnitude estimates:
15.8 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.8 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
14.8 mag. fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
14.8 mag. fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.0 (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.0d3nZCU6jA (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=25, blended=2848, bad_region=9, passed=50482
Got 50482 stars (including 47524 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 50482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 4811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 50482 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
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 50482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4811 matched stars entering correct_measured_positions(), 50482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4811 stars left (next iteration limit 5292)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=4811 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.441 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.320 n_q1=1326 n_q2=1103 n_q3=1308 n_q4=1074 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HCHmg8xxYd (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=29, blended=2904, bad_region=11, passed=50680
Got 50680 stars (including 47683 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 50680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 4816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 50680 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
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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 50680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 50680 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4815 stars left (next iteration limit 5297)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=4815 sigma_overall_arcsec=0.378 sigma_q1_arcsec=0.438 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.346 n_q1=1321 n_q2=1100 n_q3=1315 n_q4=1079 worst_quadrant_to_overall_ratio=1.160
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.EYQZkU7SDP (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=10, blended=943, bad_region=46, passed=28993
Got 28993 stars (including 27937 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat
util/solve_plate_with_UCAC5 got 28993 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.5'
Seting catalog search parameters based on the expected field of view 945.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013132 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010506 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 4812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 28993 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4823 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 28993 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 28993 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4813 stars left (next iteration limit 5293)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.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=4813 robust_rms=10.386 arcsec worst_region_rms=17.802 arcsec outer_annulus_rms=17.802 arcsec
SIP_REFIT: SIP order 3 trial: matched=4813 robust_rms=0.797 arcsec worst_region_rms=1.052 arcsec outer_annulus_rms=0.863 arcsec
SIP_REFIT: SIP order 5 trial: matched=4813 robust_rms=0.507 arcsec worst_region_rms=0.626 arcsec outer_annulus_rms=0.442 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4813 robust_rms_before=1.691 arcsec robust_rms_before_corrected=0.450 arcsec robust_rms_after=0.507 arcsec worst_region_rms_before=0.575 worst_region_rms_after=0.626 outer_annulus_rms_before=1.791 outer_annulus_rms_after=0.442
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.575 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits worst_region_rms_kept=0.575 arcsec robust_rms_kept=0.450 arcsec matched=4813
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits N_match=4813 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.558 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.499 n_q1=1524 n_q2=899 n_q3=1478 n_q4=912 worst_quadrant_to_overall_ratio=1.240
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.fCAanfXxvN (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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=6, blended=964, bad_region=43, passed=29292
Got 29292 stars (including 28234 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat
util/solve_plate_with_UCAC5 got 29292 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.3'
Seting catalog search parameters based on the expected field of view 945.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013129 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010503 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4820 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 4812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4812 matched stars entering correct_measured_positions(), 29292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 29292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 29292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4813 stars left (next iteration limit 5293)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.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=4813 robust_rms=10.540 arcsec worst_region_rms=18.293 arcsec outer_annulus_rms=18.293 arcsec
SIP_REFIT: SIP order 3 trial: matched=4813 robust_rms=0.770 arcsec worst_region_rms=1.139 arcsec outer_annulus_rms=0.852 arcsec
SIP_REFIT: SIP order 5 trial: matched=4813 robust_rms=0.493 arcsec worst_region_rms=0.634 arcsec outer_annulus_rms=0.424 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4813 robust_rms_before=1.598 arcsec robust_rms_before_corrected=0.444 arcsec robust_rms_after=0.493 arcsec worst_region_rms_before=0.574 worst_region_rms_after=0.634 outer_annulus_rms_before=1.652 outer_annulus_rms_after=0.424
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.574 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits worst_region_rms_kept=0.574 arcsec robust_rms_kept=0.444 arcsec matched=4813
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits N_match=4813 sigma_overall_arcsec=0.455 sigma_q1_arcsec=0.411 sigma_q2_arcsec=0.579 sigma_q3_arcsec=0.386 sigma_q4_arcsec=0.563 n_q1=1532 n_q2=903 n_q3=1464 n_q4=914 worst_quadrant_to_overall_ratio=1.272
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-05-57_20.00sec_-0.00C_LIGHTs_0446.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.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_2026-10-09_CI_Cnc-03-Q1b1x1_040915_TTUQ1b1x1_2390538_5N8ou92e/wcs_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447.fits
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:57:02.66 +20:16:30.7: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:09:13.10 +22:04:12.0: 12.90 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:46:26.78 +17:30:59.3: 13.18 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:13:56.00 +22:37:57.3: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:38:42.43 +21:19:11.8: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:57:02.66 +20:16:30.7: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:09:13.10 +22:04:12.0: 12.90 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry filter REJECTED candidate at 09:09:13.10 +22:04:12.0: ref_mag=12.90 +/- 0.01 new_mean_mag=12.9046 delta=-0.00 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:46:15.67 +20:36:40.0: 13.65 +/- 0.05 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:44:25.72 +16:50:37.2: 99.00 +/- 99.00 edge
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:46:26.78 +17:30:59.3: 13.13 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.16 +/- 0.02
Forced photometry filter REJECTED candidate at 08:46:26.78 +17:30:59.3: ref_mag=13.16 +/- 0.02 new_mean_mag=13.1552 delta=0.00 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:13:56.00 +22:37:57.3: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:38:42.43 +21:19:11.8: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:43:15.25 +22:04:28.7: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:46:15.67 +20:36:40.0: 13.57 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.60 +/- 0.03
Forced photometry filter REJECTED candidate at 08:46:15.67 +20:36:40.0: ref_mag=13.60 +/- 0.03 new_mean_mag=13.7292 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:44:25.72 +16:50:37.2: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 09:44:25.72 +16:50:37.2: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:13:43.89 +21:02:52.8: 14.03 +/- 0.05 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:03:29.69 +20:19:28.0: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:43:15.25 +22:04:28.7: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:13:43.89 +21:02:52.8: 13.94 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.98 +/- 0.03
Forced photometry filter REJECTED candidate at 09:13:43.89 +21:02:52.8: ref_mag=13.98 +/- 0.03 new_mean_mag=14.1419 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:03:29.69 +20:19:28.0: 16.23 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out64788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65663.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 64170_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64170_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:34:50.63 +24:27:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64178_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64178_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:28:01.29 +23:18:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64182_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64182_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 08:43:51.39 +18:22:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64183_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64183_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:47:35.97 +26:13:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64184_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64184_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 08:43:04.95 +19:27:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64648_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64648_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:09:53.95 +25:12:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64779_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64779_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:01:45.99 +17:06:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64781_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64781_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:04:57.34 +24:36:56.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64788_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
Preparing report for the candidate 64788_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
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Considering the candidate 64797_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64797_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
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Considering the candidate 64846_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64846_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
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Considering the candidate 64888_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
Preparing report for the candidate 64888_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
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Considering the candidate 64890_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
Preparing report for the candidate 64890_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
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Considering the candidate 64997_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 64997_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:02:17.58 +26:12:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65004_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65004_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:09:47.15 +25:13:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65039_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65039_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 08:54:55.83 +26:13:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65089_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65089_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:45:39.51 +23:45:05.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 65094_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65094_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:16:16.51 +23:25:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65106_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65106_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:20:35.01 +22:39:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65156_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65156_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:12:51.71 +17:27:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65173_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65173_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
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Considering the candidate 65245_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65245_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
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Considering the candidate 65252_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65252_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 08:49:21.82 +17:58:13.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65291_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65291_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:12:47.92 +20:01:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65366_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
Preparing report for the candidate 65366_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
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Considering the candidate 65389_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65389_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 08:55:05.38 +19:52:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65444_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65444_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:22:54.91 +21:56:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65633_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65633_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
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Considering the candidate 65663_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
Preparing report for the candidate 65663_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
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Considering the candidate 65675_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 65675_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:02:20.38 +20:25:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08246_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 08246_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:26:40.09 +18:37:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63831_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 63831_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
Rejecting candidate due to large distance (45.0") between the two second-epoch detections
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Considering the candidate 09229_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 09229_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
**** FOUND 09:03:15.90 +18:35:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39704_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 39704_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
Rejecting candidate due to large distance (43.1") between the two second-epoch detections
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Considering the candidate 13487_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 13487_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
Rejecting candidate due to large distance (45.0") between the two second-epoch detections
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Considering the candidate 38215_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447
The candidate 38215_fd_Cnc-03-Q1b1x1_2026-10-09_04-07-00_20.00sec_-0.00C_LIGHTs_0447 did not pass the final checks
