This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7523,10.68,0.05,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 20260408.2523 10.68CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7523,13.69,0.05,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 20260408.2523 13.69CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7523,13.84,0.05,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 20260408.2523 13.84CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7523,14.89,0.05,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 20260408.2523 14.89CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7523,13.35,0.05,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 20260408.2523 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AT Cnc,2461138.7523,13.55,0.05,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
AT Cnc 20260408.2523 13.55CV 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: 2461138.75256985 08.04.2026 06:03:32.035 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 12251
Objects passed selection criteria: 12201
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: 9139.25
Average stars matched: 8478 (92.7647 %)
Memory usage VmPeak: 116516 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 01:10:40 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: 2461138.75256985 08.04.2026 06:03:32.035 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 63
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: 30 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): 75128
Objects passed selection criteria: 74895
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: 59001.2
Average stars matched: 55007 (93.2302 %)
Memory usage VmPeak: 169240 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 01:12:11 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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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: 2461138.75203295
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits'
wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:28.196 +22:00:02.97
Angular distance between the image centers 0.0004 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:26.100 +22:00:03.02
Angular distance between the image centers 0.0082 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 08:18:28.196 +22:00:02.97
Second-epoch second image center 08:18:26.100 +22:00:03.02
Angular distance between the image centers 0.00810 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.EOLjecSkAe
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.XjC78X99O7
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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits &> /tmp/tmp.aztppMe57f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits &> /tmp/tmp.QhdMAILgVO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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: 3000)
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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
2.7 pix fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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
14.9 mag. fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
14.9 mag. fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
All-image limiting magnitude estimate: 14.9 (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.EOLjecSkAe (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.XjC78X99O7 (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.aztppMe57f (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=638, passed=10585
Got 10585 stars (including 9936 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 10585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10474 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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10474 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.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.QhdMAILgVO (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=625, passed=10501
Got 10501 stars (including 9867 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 10501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10389 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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10387 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
WARNING: Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 10387 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits'
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21084.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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 20802_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 20802_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:25:17.07 +24:20:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21084_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
Preparing report for the candidate 21084_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22451_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 22451_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:03:15.23 +20:26:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.806 670600289335196800 120.81369714356 +20.44772318471 12.3804 11.9130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
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 ####
08:18:14.31 +21:10:05.3
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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits exists and is non-empty
wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:28.196 +22:00:02.97
Angular distance between the image centers 0.0004 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.231 +22:00:01.67
Second-epoch image center 08:18:26.100 +22:00:03.02
Angular distance between the image centers 0.0082 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 08:18:28.196 +22:00:02.97
Second-epoch second image center 08:18:26.100 +22:00:03.02
Angular distance between the image centers 0.00810 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.zsiOBvZi3w
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.FkX8oSrCYr
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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits &> /tmp/tmp.gEVRRynOIN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits &> /tmp/tmp.Z63p9KAlJ9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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 45 candidate transients before the final filtering. (Hard limit: 3000)
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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
2.3 pix fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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
15.1 mag. fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
15.1 mag. fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.6 (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.zsiOBvZi3w (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.FkX8oSrCYr (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.gEVRRynOIN (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3624, passed=60427
Got 60427 stars (including 56746 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 60427 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 59845 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 16.5 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
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 59845 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 59845 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.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.Z63p9KAlJ9 (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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=3576, passed=60187
Got 60187 stars (including 56552 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 60187 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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...
WARNING: Accuracy estimation diagnostic: 974 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...
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 59597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 59597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
WARNING: Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 59597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/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_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-02-45_20.00sec_-4.90C_LIGHT_0064.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.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_2026-04-08_CI_Cnc-02-Q2b1x1_010420_TTUQ2b1x1_20317_mo0Lyx90/wcs_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065.fits
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out104903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out104325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out108830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40496.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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 99794_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99794_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:19:07.03 +21:47:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.216 676420897734346624 124.77916220676 +21.79431574780 15.0859 14.5412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99797_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99797_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:07:46.58 +23:03:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.649 680220638121452544 121.94446379338 +23.05326747021 14.9082 14.3853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99804_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99804_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:07:42.52 +18:27:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 0.801 668994933639633792 121.92696057846 +18.45844923444 14.7739 14.2569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99805_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99805_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:10:06.44 +22:40:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 0.698 677144479464617088 122.52702282073 +22.66741641652 14.5741 14.1360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99809_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99809_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:23:02.74 +22:37:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.174 676571599546881792 125.76076544829 +22.62644596392 14.4918 13.8353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99810_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99810_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:11:05.73 +18:22:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 1.720 657344302273552640 122.77411013213 +18.37435535160 14.6268 14.1201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99811_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99811_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:05:19.55 +21:11:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 0.428 670934094193508992 121.33158343235 +21.18871749712 14.0666 13.5005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99819_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99819_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:04:45.75 +20:40:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.249 670704364982787072 121.19063746265 +20.67990156645 14.7112 14.1259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99820_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99820_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:10:56.15 +23:35:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.456 677614658124639744 122.73406565753 +23.58680898337 14.1991 13.5980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99822_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99822_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:14:26.53 +21:45:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.520 676092521714626176 123.61063063308 +21.76535371594 14.1751 13.6758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99823_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99823_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:26:17.81 +22:51:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.841 677904104560602368 126.57432366713 +22.86345795084 13.9218 13.3744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99824_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99824_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:14:15.89 +17:57:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.708 657092857709090304 123.56610317108 +17.96544167611 13.7861 13.1109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99828_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99828_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:12:44.18 +23:01:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 0.303 677524532531091584 123.18405024946 +23.02068944395 13.7328 12.9332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99831_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 99831_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:02:03.55 +24:56:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100349_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 100349_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:18:14.32 +21:10:05.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 103281_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 103281_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:00:22.36 +25:02:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103416_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 103416_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:07:25.72 +19:47:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103945_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 103945_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:06:22.96 +24:01:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104096_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 104096_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:33:21.09 +20:21:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104325_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
Preparing report for the candidate 104325_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
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Considering the candidate 104903_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 104903_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:02:38.94 +22:39:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.054 680127591950073216 120.66193320942 +22.65179558303 14.0228 13.6087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104969_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
Preparing report for the candidate 104969_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
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Considering the candidate 105156_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 105156_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:13:35.56 +23:07:38.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105273_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 105273_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:10:29.11 +25:31:52.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105296_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 105296_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:08:57.26 +24:37:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105696_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 105696_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 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 106064_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 106064_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:17:00.97 +18:29:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.937 657228509955087360 124.25359558830 +18.49799917018 14.2133 13.7327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106095_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 106095_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:14:11.46 +24:34:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.372 680793140081790336 123.54774242961 +24.57346416312 14.2571 13.8335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106182_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 106182_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:20:26.37 +23:17:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.463 677416264994942208 125.10981165215 +23.29069802447 14.1888 13.5715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106502_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 106502_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:17:15.51 +21:38:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106612_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 106612_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:08:23.95 +22:51:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.609 677188803527023104 122.09972916390 +22.86006316527 14.3077 13.8028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106710_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 106710_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:29:47.80 +20:47:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107091_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 107091_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:06:10.74 +25:28:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107162_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 107162_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:15:44.01 +18:56:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107396_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 107396_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:10:32.46 +24:41:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107776_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 107776_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:00:12.58 +23:04:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 0.429 680350483572599168 120.05245109147 +23.07744814724 14.8469 14.3893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107899_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 107899_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:01:25.40 +24:23:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 2.922 681327154838913408 120.35538949380 +24.39226824105 14.5804 13.7322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108083_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 108083_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:15:51.99 +18:13:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 0.870 657195077929687936 123.96652729065 +18.22916762417 14.9839 14.4741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108151_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 108151_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:11:43.68 +23:27:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 0.680 677621358273615744 122.93203185965 +23.45685335352 14.7773 14.2813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108548_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 108548_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:07:32.20 +22:15:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.717 677062359689867520 121.88396081941 +22.25563172636 15.0477 14.6328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108821_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 108821_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks
**** FOUND 08:10:24.96 +18:34:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 0.969 669360555615552640 122.60407305157 +18.57020460199 14.6766 13.9632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108830_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
Preparing report for the candidate 108830_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
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Considering the candidate 108875_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065
The candidate 108875_fd_Cnc-02-Q2b1x1_2026-04-08_01-03-32_20.00sec_-4.90C_LIGHT_0065 did not pass the final checks