This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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,2461147.6984,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1984 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
target,2461147.6984,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1984 13.81CV 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
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
target,2461147.6984,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1984 13.72CV 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
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
ATO J130.0408+18.0971,2461147.6984,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J130.0408+18.0971 20260417.1984 13.26CV 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
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,2461147.6984,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1984 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
ASAS J084138+1619.8,2461147.6984,7.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J084138+1619.8 20260417.1984 7.97CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
First image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Last image: 2461147.69868065 17.04.2026 04:45:56.008 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9430
Objects passed selection criteria: 9391
Measurements per detected object (mean, median, min, max): 3.0 2.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 2.0 2 4
Average stars detected per image: 7215.5
Average stars matched: 6558 (90.8877 %)
Memory usage VmPeak: 113936 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 23:49:36 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: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
First image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Last image: 2461147.69868065 17.04.2026 04:45:56.008 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 61
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 55004
Objects passed selection criteria: 54807
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 40007.2
Average stars matched: 37062 (92.6382 %)
Memory usage VmPeak: 152496 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 23:50:34 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461147.69814700
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-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits (1st reference image)
verification OK: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:53:20.681 +13:59:51.92 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-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits (1st new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Image size: 936.7'x623.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:22.901 +13:59:24.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:22.901 +13:59:24.39
Angular distance between the image centers 0.0118 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits (2nd new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 936.7'x623.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:23.620 +13:59:29.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:23.620 +13:59:29.41
Angular distance between the image centers 0.0134 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 08:53:22.901 +13:59:24.39
Second-epoch second image center 08:53:23.620 +13:59:29.41
Angular distance between the image centers 0.00322 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits &> /tmp/tmp.vEm4kN5KWl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits &> /tmp/tmp.GVgbxVSZlT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits &> /tmp/tmp.BGPIbbZwER
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits &> /tmp/tmp.65PYyfN7oZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat' -> 'wcsmag.cat'
Read 9772 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 124.9313 to 141.4877 deg, Dec +8.4819 to +19.3313 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 124.9313 to 141.4877 deg, Dec 8.4819 to 19.3313 deg
Loaded 7052 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): 5574 out of 5900 total matches.
Matched with Tycho-2 5900 out of 9772 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.809505
a=0.000000 b=1.000000 c=22.809505
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
2.0 pix Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
4.0 pix fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
3.9 pix fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Limiting magnitude estimates:
15.2 mag. Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
15.2 mag. Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
14.3 mag. fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
14.3 mag. fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.vEm4kN5KWl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, passed=9772
Got 9772 stars (including 8997 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
util/solve_plate_with_UCAC5 got 9772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 9575 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 9576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 9576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GVgbxVSZlT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=774, passed=9656
Got 9656 stars (including 8873 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 9656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9493 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9491 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 9491 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.BGPIbbZwER (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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1145, passed=8449
Got 8449 stars (including 7302 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 8449 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 8093 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 8092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 8092 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.65PYyfN7oZ (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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1106, passed=8405
Got 8405 stars (including 7298 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 8405 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 8068 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 8070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 8070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits'
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21279.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21279_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
Preparing report for the candidate 21279_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21963_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 21963_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 09:01:15.99 +11:57:52.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21983_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 21983_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:54:14.96 +14:44:20.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22128_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 22128_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:54:38.59 +11:34:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 1.175 604717342143816064 133.66088791555 +11.57253478179 12.2578 11.8456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22129_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 22129_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 09:04:32.24 +12:52:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22146_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 22146_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 09:08:42.53 +15:11:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.709 607705264992398848 137.17741244336 +15.18344853108 12.3590 11.7427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22182_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 22182_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:58:25.64 +18:13:41.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01958_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 01958_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:56:58.98 +10:51:12.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:01:11.19 +10:09:46.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits exists and is non-empty
wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits (1st reference image)
verification OK: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:53:20.681 +13:59:51.92 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-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits (1st new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Image size: 936.7'x623.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:22.901 +13:59:24.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:22.901 +13:59:24.39
Angular distance between the image centers 0.0118 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits (2nd new image)
verification OK: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Image size: 936.7'x623.8' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:53:23.620 +13:59:29.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:23.620 +13:59:29.41
Angular distance between the image centers 0.0134 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 08:53:22.901 +13:59:24.39
Second-epoch second image center 08:53:23.620 +13:59:29.41
Angular distance between the image centers 0.00322 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits &> /tmp/tmp.vNB4iF156O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits &> /tmp/tmp.KcIZfFFxZj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits &> /tmp/tmp.43oiU0eDn2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits &> /tmp/tmp.DZISwhWA0a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat' -> 'wcsmag.cat'
Read 61604 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 124.9313 to 141.4942 deg, Dec +8.4527 to +19.3337 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 124.9313 to 141.4942 deg, Dec 8.4527 to 19.3337 deg
Loaded 7075 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): 5222 out of 6038 total matches.
Matched with Tycho-2 6038 out of 61604 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.669299
a=0.000000 b=1.000000 c=22.669299
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 34 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.8 pix Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
1.8 pix Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
3.7 pix fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
3.7 pix fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Limiting magnitude estimates:
15.4 mag. Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
15.4 mag. Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
14.8 mag. fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
14.8 mag. fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.vNB4iF156O (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3469, passed=61585
Got 61585 stars (including 58012 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
util/solve_plate_with_UCAC5 got 61585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 60529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 60529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 60529 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.KcIZfFFxZj (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3459, passed=61573
Got 61573 stars (including 57999 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 61573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 60538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 60537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 60538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.43oiU0eDn2 (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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=5642, passed=35067
Got 35067 stars (including 29411 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 35067 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 33337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 33338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 33338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.DZISwhWA0a (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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=5643, passed=35234
Got 35234 stars (including 29570 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 35234 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.7'
Seting catalog search parameters based on the expected field of view 936.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013010 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010408 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 33703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 33705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 33705 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-09_20.00sec_-4.90C_LIGHT_0119.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.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_2026-04-16_CI_Cnc-05-Q2b1x1_234644_TTUQ2b1x1_51088_NkVhcvuZ/wcs_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120.fits
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out75505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out56194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80317.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 75497_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
Preparing report for the candidate 75497_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
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Considering the candidate 75505_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 75505_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:40:17.97 +11:38:07.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)
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Considering the candidate 75506_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
Preparing report for the candidate 75506_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
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Considering the candidate 75517_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
Preparing report for the candidate 75517_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
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Considering the candidate 76459_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 76459_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 09:01:11.19 +10:09:46.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 77111_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 77111_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 77621_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 77621_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 77997_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 77997_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 78962_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 78962_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:49:32.68 +12:08:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79383_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 79383_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 79825_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 79825_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 79958_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 79958_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 80118_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 80118_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:43:09.11 +14:05:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80317_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
Preparing report for the candidate 80317_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
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Considering the candidate 80715_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 80715_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:49:56.26 +14:48:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82522_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 82522_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 82598_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 82598_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 56194_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
Preparing report for the candidate 56194_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
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Considering the candidate 11026_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 11026_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:56:58.97 +10:51:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48896_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 48896_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:51:01.22 +15:21:04.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21395_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 21395_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:48:39.58 +12:32:51.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 42574_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 42574_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:57:14.85 +15:19:20.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 08725_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 08725_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:48:37.16 +10:26:01.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 60773_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 60773_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:57:35.13 +15:34:51.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12544_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 12544_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:40:32.64 +10:55:28.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 19578_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 19578_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:46:55.97 +12:06:36.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15929_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 15929_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:55:55.38 +11:37:38.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17225_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 17225_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:58:29.03 +11:51:32.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23114_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 23114_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:43:12.50 +12:40:53.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 61426_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 61426_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:36:07.81 +15:18:49.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 51332_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 51332_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:55:22.79 +17:13:48.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 07406_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 07406_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:44:45.07 +10:04:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 45538_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 45538_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks
**** FOUND 08:44:41.30 +18:09:03.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 05384_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120
The candidate 05384_fd_Cnc-05-Q2b1x1_2026-04-16_23-45-56_20.00sec_-5.00C_LIGHT_0120 did not pass the final checks