This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.6912,10.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1912 10.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461147.6912,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260417.1912 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.6912,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1912 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.6912,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1912 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.6912,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1912 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.6912,14.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1912 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.6912,14.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1912 14.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.6912,14.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.1912 14.84CV 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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461147.69149505 17.04.2026 04:35:35.172 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 4 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): 12318
Objects passed selection criteria: 12255
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 9340
Average stars matched: 8659 (92.7088 %)
Memory usage VmPeak: 116516 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 23:42:51 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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Last image: 2461147.69149505 17.04.2026 04:35:35.172 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 72
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
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: 25 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): 76062
Objects passed selection criteria: 75801
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 60214.2
Average stars matched: 56161.2 (93.269 %)
Memory usage VmPeak: 170684 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 16 23:44:01 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
SExtractor catalog cache: saved Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461147.69093323
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
Saving wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits to local_wcs_cache/
'wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
Saving wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits to local_wcs_cache/
'wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits'
wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits (1st reference image)
verification OK: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:28.231 +22:00:01.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits (1st new image)
verification OK: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:18:36.092 +21:59:07.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:36.092 +21:59:07.05
Angular distance between the image centers 0.0340 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits (2nd new image)
verification OK: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:18:35.587 +21:58:34.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:35.587 +21:58:34.29
Angular distance between the image centers 0.0374 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 08:18:36.092 +21:59:07.05
Second-epoch second image center 08:18:35.587 +21:58:34.29
Angular distance between the image centers 0.00931 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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.hR9Tdtipbz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.8XqUnNziQP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits &> /tmp/tmp.70wMSDhSk7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits &> /tmp/tmp.6jARVBST3Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Cnc-02-Q2b1x1_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: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
2.1 pix Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.7 pix fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
2.7 pix fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Limiting magnitude estimates:
15.4 mag. Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
15.4 mag. Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
15.0 mag. fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
15.0 mag. fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.0 (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.hR9Tdtipbz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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.8XqUnNziQP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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.70wMSDhSk7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=695, passed=11137
Got 11137 stars (including 10432 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat
util/solve_plate_with_UCAC5 got 11137 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
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(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 532 to 588 (Dec 16.5 to 27.3)
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(), 11026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.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.6jARVBST3Y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=706, passed=11089
Got 11089 stars (including 10376 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat
util/solve_plate_with_UCAC5 got 11089 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
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(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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 532 to 588 (Dec 16.4 to 27.3)
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(), 10964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 10964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
Saving fully-calibrated image wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits'
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21107.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20835_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 20835_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:25:17.06 +24:20:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21107_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 21107_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21506_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 21506_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:04:51.59 +23:37:18.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:28:35.07 +20:44:07.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
SExtractor catalog cache: saved Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Creating symlink local_wcs_cache/wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits exists and is non-empty
wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits (1st reference image)
verification OK: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:18:28.231 +22:00:01.67 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits (1st new image)
verification OK: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:18:36.092 +21:59:07.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:36.092 +21:59:07.05
Angular distance between the image centers 0.0340 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits (2nd new image)
verification OK: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 08:18:35.587 +21:58:34.29 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:35.587 +21:58:34.29
Angular distance between the image centers 0.0374 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 08:18:36.092 +21:59:07.05
Second-epoch second image center 08:18:35.587 +21:58:34.29
Angular distance between the image centers 0.00931 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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits &> /tmp/tmp.40EQ3JpAfF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits &> /tmp/tmp.5pJw7GAKyx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits &> /tmp/tmp.U0dkk9aksg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits &> /tmp/tmp.bxLdEOXuwj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
Found non-empty wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits and wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
The reference image (wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits) and catalog (wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat) found
'wcs_Cnc-02-Q2b1x1_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.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 55 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
1.9 pix Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
2.3 pix fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
2.2 pix fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Limiting magnitude estimates:
15.6 mag. Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
15.6 mag. Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
15.2 mag. fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
15.2 mag. fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.7 (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.40EQ3JpAfF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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.5pJw7GAKyx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_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=25, blended=6314, passed=84332
Got 84332 stars (including 77878 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 84332 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 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(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 83178 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 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(), 83179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 83179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q2b1x1_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-Q2b1x1_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.U0dkk9aksg (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=4069, passed=63600
Got 63600 stars (including 59462 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat
util/solve_plate_with_UCAC5 got 63600 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
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(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 62855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 532 to 588 (Dec 16.4 to 27.3)
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(), 62855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 62855 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.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.bxLdEOXuwj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=4110, passed=63797
Got 63797 stars (including 59616 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat
util/solve_plate_with_UCAC5 got 63797 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
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(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 63071 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 532 to 588 (Dec 16.4 to 27.3)
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(), 63070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 63070 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.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-Q2b1x1_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_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Saving fully-calibrated image wcs_Cnc-02-Q2b1x1_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_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-34-46_20.00sec_-5.00C_LIGHT_0111.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-16_CI_Cnc-02-Q2b1x1_233614_TTUQ2b1x1_3644203_ikZDTi8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112.fits
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out106910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out102484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out99813.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 99803_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99803_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:34:43.31 +24:05:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99805_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99805_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:04:19.47 +23:04:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.440 680165799979068672 121.08099204991 +23.06719381791 15.0404 14.5811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99806_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99806_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:06:56.74 +19:33:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.270 669736726031254656 121.73648476618 +19.56262218189 14.5036 13.9190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99813_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 99813_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
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Considering the candidate 99814_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99814_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:05:51.60 +20:04:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99818_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99818_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:27:35.41 +26:01:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99819_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99819_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:12:45.95 +20:07:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.835 675633303811652992 123.19135451141 +20.11822266030 14.2514 13.3891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99821_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99821_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:14:44.31 +21:25:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99822_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99822_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:10:56.16 +23:35:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99824_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99824_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:14:26.57 +21:45:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99828_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99828_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:12:44.14 +23:01:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99829_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99829_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:14:15.88 +17:57:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99834_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99834_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:23:50.98 +23:10:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99835_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99835_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:02:03.49 +24:56:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99839_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 99839_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:09:57.99 +23:29:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100403_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 100403_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:28:35.07 +20:44:07.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 102484_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 102484_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
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Considering the candidate 103035_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 103035_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:07:25.72 +19:47:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103235_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 103235_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:00:22.32 +25:02:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103713_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 103713_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
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Considering the candidate 103858_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 103858_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:13:01.49 +25:18:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104493_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 104493_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
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Considering the candidate 104924_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 104924_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:02:38.95 +22:39:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105122_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105122_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:17:00.89 +18:29:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105206_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105206_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:19:28.76 +22:27:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105331_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105331_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:23:23.69 +21:50:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105337_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105337_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:13:35.56 +23:07:39.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105751_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105751_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:13:55.69 +21:21:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105779_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105779_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:20:26.37 +23:17:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105835_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105835_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:08:23.99 +22:51:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105842_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 105842_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
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Considering the candidate 105909_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 105909_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:10:34.71 +25:30:30.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106103_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 106103_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:15:44.02 +18:56:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106510_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 106510_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:06:10.63 +25:28:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106563_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 106563_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:24:21.04 +18:55:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106611_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 106611_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:10:32.61 +24:41:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106740_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 106740_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:24:36.40 +19:41:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106862_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 106862_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
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Considering the candidate 106910_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 106910_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:05:34.95 +20:26:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 1.786 670637810169573760 121.39546174828 +20.44419479718 14.7591 14.2681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106932_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 106932_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:01:25.44 +24:23:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107051_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 107051_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:05:52.77 +18:29:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107073_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 107073_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:06:33.52 +21:14:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107422_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 107422_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:23:02.62 +22:37:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107477_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 107477_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:11:43.73 +23:27:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108176_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108176_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:29:34.39 +19:16:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 0.869 662902707211762944 127.39323672310 +19.27984761571 15.0457 14.3570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108417_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108417_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:15:12.98 +24:56:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.500 682309847652770560 123.80402474231 +24.94370508957 15.1637 14.6255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108544_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108544_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:10:24.98 +18:34:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108574_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108574_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:23:53.54 +20:03:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108679_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108679_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:27:46.71 +22:52:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.844 677860089735816448 126.94437067293 +22.87000093754 14.8631 14.1485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108688_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108688_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:16:51.41 +18:58:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108724_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108724_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:10:30.62 +25:33:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108745_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108745_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:16:16.50 +18:27:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108873_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108873_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
**** FOUND 08:14:50.05 +21:36:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108883_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
Preparing report for the candidate 108883_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
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Considering the candidate 108948_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112
The candidate 108948_fd_Cnc-02-Q2b1x1_2026-04-16_23-35-35_20.00sec_-4.90C_LIGHT_0112 did not pass the final checks
