This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO
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
Gaia DR3 664109077626584064,2461143.7310,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 664109077626584064 20260413.2310 10.40CV 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,2461143.7310,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2310 12.80CV 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,2461143.7310,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2310 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461143.7310,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2310 13.40CV 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,2461143.7310,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2310 13.63CV 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,2461143.7310,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2310 13.71CV 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,2461143.7310,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2310 14.01CV 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,2461143.7310,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.2310 14.48CV 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 J081756+2327.3,2461143.7310,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J081756+2327.3 20260413.2310 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.70008337 22.02.2026 04:47:57.203 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
First image: 2461093.70008337 22.02.2026 04:47:57.203 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461143.73145071 13.04.2026 05:33:07.341 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 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): 13290
Objects passed selection criteria: 13251
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 10901.5
Average stars matched: 10635 (97.5554 %)
Memory usage VmPeak: 118148 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:36:59 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.70008337 22.02.2026 04:47:57.203 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
First image: 2461093.70008337 22.02.2026 04:47:57.203 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461143.73145071 13.04.2026 05:33:07.341 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 39
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 19 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): 79852
Objects passed selection criteria: 79662
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 67331.5
Average stars matched: 65007 (96.5477 %)
Memory usage VmPeak: 2783504 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 00:38:04 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.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: 2461143.73052141
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
Saving wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
Saving wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits'
wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:24.533 +22:02:48.69
Angular distance between the image centers 0.0485 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:22.234 +22:03:18.94
Angular distance between the image centers 0.0595 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 08:18:24.533 +22:02:48.69
Second-epoch second image center 08:18:22.234 +22:03:18.94
Angular distance between the image centers 0.01222 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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.RkxyST9dzX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.8q1rovJ2q3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits &> /tmp/tmp.IWI4GWGY3G
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits &> /tmp/tmp.o1zWlaUlmR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat' -> 'wcsmag.cat'
Read 13703 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6698 to 133.2123 deg, Dec +16.3190 to +27.3485 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 115.6698 to 133.2123 deg, Dec 16.3190 to 27.3485 deg
Loaded 8739 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): 6706 out of 7190 total matches.
Matched with Tycho-2 7190 out of 13703 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.921568
a=0.000000 b=1.000000 c=22.921568
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
2.1 pix Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.2 pix fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
2.2 pix fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Limiting magnitude estimates:
15.4 mag. Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
15.4 mag. Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
14.7 mag. fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
14.7 mag. fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.RkxyST9dzX (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1104, passed=13703
Got 13703 stars (including 12580 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 13703 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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13448 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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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.8q1rovJ2q3 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1109, passed=13640
Got 13640 stars (including 12518 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 13640 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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13354 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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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.IWI4GWGY3G (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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=550, passed=8821
Got 8821 stars (including 8261 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat
util/solve_plate_with_UCAC5 got 8821 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 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 8709 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.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.o1zWlaUlmR (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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=480, passed=7683
Got 7683 stars (including 7193 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat
util/solve_plate_with_UCAC5 got 7683 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 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 7371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 7371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 7371 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
Saving fully-calibrated image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits'
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20732.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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20698_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 20698_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:25:17.03 +24:20:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20732_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 20732_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00776_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 00776_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:21:42.81 +17:17:06.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:23:48.43 +20:56:45.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:24.533 +22:02:48.69
Angular distance between the image centers 0.0485 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:22.234 +22:03:18.94
Angular distance between the image centers 0.0595 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 08:18:24.533 +22:02:48.69
Second-epoch second image center 08:18:22.234 +22:03:18.94
Angular distance between the image centers 0.01222 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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.3r57xWjyAm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.t6bQApxYds
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits &> /tmp/tmp.WXjGPF1oua
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits &> /tmp/tmp.4uoUfcU6FW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat' -> 'wcsmag.cat'
Read 84194 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 115.6500 to 133.2207 deg, Dec +16.3111 to +27.3510 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 115.6500 to 133.2207 deg, Dec 16.3111 to 27.3510 deg
Loaded 8767 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): 5951 out of 7242 total matches.
Matched with Tycho-2 7242 out of 84194 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.789886
a=0.000000 b=1.000000 c=22.789886
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 36 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
1.9 pix Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.2 pix fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
2.0 pix fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Limiting magnitude estimates:
15.5 mag. Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
15.5 mag. Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
14.8 mag. fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
14.8 mag. fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.3r57xWjyAm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=6351, passed=84160
Got 84160 stars (including 77670 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 84160 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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82903 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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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.t6bQApxYds (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=6314, passed=84327
Got 84327 stars (including 77873 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 84327 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 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 83173 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 83174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 83174 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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.WXjGPF1oua (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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2773, passed=53789
Got 53789 stars (including 50945 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat
util/solve_plate_with_UCAC5 got 53789 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 53164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 53164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 53164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.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.4uoUfcU6FW (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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2462, passed=48897
Got 48897 stars (including 46362 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat
util/solve_plate_with_UCAC5 got 48897 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 530 to 590 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 46969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 590 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 46970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 46970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.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-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_Cnc-02-Q1b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Saving fully-calibrated image wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_Cnc-02-Q1b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-31-47_20.00sec_-4.90C_LIGHTs_0054.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.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_2026-04-13_CI_Cnc-02-Q1b1x1_003358_TTUQ1b1x1_15463_HPAFeRwO/wcs_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055.fits
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out100675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84047.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100675_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100675_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:37:09.01 +24:16:08.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100676_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100676_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:13:52.39 +25:25:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 2.421 682394784925792768 123.46770180954 +25.42643815876 15.0270 14.5201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100690_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100690_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:14:26.55 +21:45:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100691_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100691_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100692_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100692_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:50:04.70 +19:56:50.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100693_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100693_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:26:17.82 +22:51:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100695_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100695_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:37:28.40 +24:00:32.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100698_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100698_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:10:33.65 +19:11:20.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100783_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 100783_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:23:48.43 +20:56:45.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101097_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 101097_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 07:54:54.76 +24:09:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101464_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 101464_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101623_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 101623_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:07:25.70 +19:47:40.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101690_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 101690_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:43:57.56 +19:01:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101747_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 101747_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:00:22.31 +25:02:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101755_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 101755_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101832_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 101832_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101853_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 101853_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:02:03.49 +24:56:57.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101957_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 101957_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:43:42.89 +16:53:19.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101989_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 101989_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:32:53.27 +18:33:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101999_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 101999_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102120_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102120_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:38:50.69 +23:40:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102123_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 102123_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102138_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102138_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:02:38.97 +22:39:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102170_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102170_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:10:29.23 +25:31:54.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102202_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102202_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 07:52:14.33 +21:09:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102294_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102294_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:12:44.17 +23:01:13.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102295_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102295_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:10:10.10 +27:04:09.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102303_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102303_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:31:17.07 +19:12:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102390_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102390_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:37:41.73 +19:46:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102434_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102434_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:23:23.70 +21:50:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102512_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102512_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:10:56.14 +23:35:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102592_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 102592_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102811_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 102811_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
**** FOUND 08:52:35.95 +23:59:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102937_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
Preparing report for the candidate 102937_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03987_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055
The candidate 03987_fd_Cnc-02-Q1b1x1_2026-04-13_00-33-07_20.00sec_-4.90C_LIGHTs_0055 did not pass the final checks
