This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.7169,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.2169 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.7169,13.46,0.05,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 20260410.2169 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.7169,13.64,0.05,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 20260410.2169 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.7169,14.04,0.05,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 20260410.2169 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461140.7169,14.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.2169 14.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AS Cnc,2461140.7169,12.00,0.05,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
AS Cnc 20260410.2169 12.00CV 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: 2461140.71714037 10.04.2026 05:12:30.928 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
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): 12462
Objects passed selection criteria: 12405
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: 9427.25
Average stars matched: 8724.25 (92.5429 %)
Memory usage VmPeak: 116520 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 00:23:41 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: 2461140.71714037 10.04.2026 05:12:30.928 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
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: 31 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): 76719
Objects passed selection criteria: 76462
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: 60818.8
Average stars matched: 56622.5 (93.1004 %)
Memory usage VmPeak: 1924292 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 00:25:10 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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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: 2461140.71656821
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits exists and is non-empty
Saving wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits to local_wcs_cache/
'wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits exists and is non-empty
Saving wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits to local_wcs_cache/
'wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits'
wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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 08:18:47.109 +21:59:29.72
Angular distance between the image centers 0.0735 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 08:18:49.224 +21:59:04.14
Angular distance between the image centers 0.0827 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 08:18:47.109 +21:59:29.72
Second-epoch second image center 08:18:49.224 +21:59:04.14
Angular distance between the image centers 0.01083 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.Kt7zqp9XQV
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.OkYg0bBnp9
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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits &> /tmp/tmp.Pmis3haMKv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits &> /tmp/tmp.AxhuUmLtTa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
2.7 pix fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
Limiting magnitude estimates:
15.4 mag. Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
15.4 mag. Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
15.0 mag. fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
15.0 mag. fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (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.Kt7zqp9XQV (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1104, passed=13703
Got 13703 stars (including 12580 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 13703 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13448 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 13450 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OkYg0bBnp9 (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1109, passed=13640
Got 13640 stars (including 12518 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 13640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 13355 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Pmis3haMKv (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=739, passed=11513
Got 11513 stars (including 10765 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 11513 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11397 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11398 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.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.AxhuUmLtTa (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=749, passed=11527
Got 11527 stars (including 10767 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat
util/solve_plate_with_UCAC5 got 11527 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11431 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 11429 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
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_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits'
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21013.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21013_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
Preparing report for the candidate 21013_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21515_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 21515_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:04:51.58 +23:37:18.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22049_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 22049_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:25:42.23 +25:43:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.556 679611371240857216 126.42579069430 +25.71900388915 12.5748 12.1761 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#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: 6s
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 ####
08:20:22.52 +21:05:10.3
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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits exists and is non-empty
wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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 08:18:47.109 +21:59:29.72
Angular distance between the image centers 0.0735 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 08:18:49.224 +21:59:04.14
Angular distance between the image centers 0.0827 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 08:18:47.109 +21:59:29.72
Second-epoch second image center 08:18:49.224 +21:59:04.14
Angular distance between the image centers 0.01083 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.rwvLrcKRca
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.kfjCFWfJr4
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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits &> /tmp/tmp.eYZdH0XVcH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits &> /tmp/tmp.omFDj2JvVZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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 52 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
2.2 pix fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
2.2 pix fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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
15.3 mag. fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
15.3 mag. fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rwvLrcKRca (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits' -> 'wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=6351, passed=84160
Got 84160 stars (including 77670 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat
util/solve_plate_with_UCAC5 got 84160 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 82903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits -region wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-47-57_20.00sec_-15.00C_LIGHT_0173.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kfjCFWfJr4 (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits' -> 'wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS-calibrated image found: wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
Checking if the catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat corresponding to the image wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits
WCS catalog name: wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=6314, passed=84332
Got 84332 stars (including 77878 good ones) from the SExtractor catalog wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat
util/solve_plate_with_UCAC5 got 84332 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 83178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 83179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 83179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits -region wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q2b1x1_2026-02-21_22-48-51_20.00sec_-15.00C_LIGHT_0174.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eYZdH0XVcH (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=4388, passed=65298
Got 65298 stars (including 60846 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 65298 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 64521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 64521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 64521 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.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.omFDj2JvVZ (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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
Checking if the catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat corresponding to the image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
WCS catalog name: wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=4393, passed=65355
Got 65355 stars (including 60893 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat
util/solve_plate_with_UCAC5 got 65355 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 64571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 64570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 64571 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits -region wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/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_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-11-41_20.00sec_-5.00C_LIGHT_0092.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.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_2026-04-10_CI_Cnc-02-Q2b1x1_001309_TTUQ2b1x1_24521_DVjFUN8m/wcs_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093.fits
Preparing the HTML report for the field Cnc-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out102412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out99836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out99819.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out103456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66250.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 99802_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99802_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:15:12.91 +18:16:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.316 657385396521303168 123.80388407352 +18.27105319374 14.6511 14.1352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99807_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99807_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:24:27.54 +22:10:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 0.772 676310087582269824 126.11476307973 +22.17115841672 14.6653 14.1509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99809_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99809_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:10:06.51 +22:40:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99812_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99812_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:07:42.52 +18:27:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99816_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99816_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:23:02.70 +22:37:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99817_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99817_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:12:45.42 +20:06:48.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.265 675633063293355904 123.18914027407 +20.11386367446 14.3561 14.0609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99819_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99819_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:09:18.38 +19:30:00.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 99821_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99821_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:14:26.59 +21:45:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99825_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99825_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:26:17.84 +22:51:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99827_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99827_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:10:56.12 +23:35:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99828_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99828_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:20:26.44 +23:17:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99829_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99829_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:09:46.93 +25:51:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.254 682666158139442816 122.44540717119 +25.85372899320 14.3442 13.8777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99830_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99830_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:30:13.35 +23:13:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.437 677975641541260160 127.55572996417 +23.22440710595 13.8045 13.3021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 99831_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99831_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:27:35.17 +26:01:55.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)
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Considering the candidate 99832_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99832_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:12:44.15 +23:01:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99833_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99833_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:14:15.82 +17:57:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99835_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99835_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:37:28.55 +24:00:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99836_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99836_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:13:50.27 +20:30:50.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 99837_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99837_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:02:03.49 +24:56:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99841_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 99841_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:33:35.53 +18:17:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100298_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 100298_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:20:22.52 +21:05:10.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 102412_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 102412_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:18:43.14 +21:35:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.046 676393753541050752 124.67960309929 +21.59733971683 12.9983 12.5442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.046#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103133_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 103133_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:07:25.69 +19:47:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103146_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 103146_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:00:22.33 +25:02:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103456_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
Preparing report for the candidate 103456_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
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Considering the candidate 103649_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 103649_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:06:22.96 +24:01:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104001_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
Preparing report for the candidate 104001_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
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Considering the candidate 105160_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 105160_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:02:38.88 +22:39:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105283_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 105283_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:19:28.80 +22:27:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.661 676597953466184064 124.86997272874 +22.45654290066 14.3740 13.9280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 105325_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 105325_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:13:35.56 +23:07:39.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105522_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
Preparing report for the candidate 105522_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
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Considering the candidate 105956_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 105956_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:10:34.63 +25:30:30.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106292_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 106292_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:15:44.08 +18:57:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106659_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 106659_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:31:24.28 +18:25:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.480 662610275775934848 127.85077004258 +18.42102638525 14.1272 13.7001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106724_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 106724_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:12:17.86 +18:16:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106823_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 106823_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:17:15.49 +21:38:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106847_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 106847_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:01:25.42 +24:23:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106998_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 106998_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:24:21.14 +18:55:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107341_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 107341_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:10:32.42 +24:41:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107351_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 107351_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:05:52.85 +18:29:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.481 669050287178069120 121.46968314045 +18.48642071090 14.8160 14.3940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107714_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 107714_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:01:43.18 +22:50:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107732_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 107732_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:11:43.70 +23:27:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107909_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
Preparing report for the candidate 107909_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
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Considering the candidate 108219_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 108219_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:14:20.58 +21:02:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108311_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 108311_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:08:57.04 +22:16:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108415_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 108415_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:06:33.61 +21:14:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.337 670752674774784256 121.64013538681 +21.23547824853 14.8779 14.3515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108782_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 108782_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:03:45.33 +19:46:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 0.429 670482160554940800 120.93889795886 +19.77053394620 15.0843 14.4664 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 108792_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 108792_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:11:16.70 +19:30:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.662 669573620352863360 122.81975922249 +19.51350379529 14.8222 14.2126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108866_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 108866_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:16:43.42 +17:45:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109115_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 109115_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks
**** FOUND 08:11:02.02 +19:41:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 0.887 669592273394781824 122.75866079568 +19.69853351057 15.0769 14.6207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109198_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093
The candidate 109198_fd_Cnc-02-Q2b1x1_2026-04-10_00-12-30_20.00sec_-5.00C_LIGHT_0093 did not pass the final checks