This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.2770 2461126.7770 14.12 14:01:41.82 +33:49:22.2
61.09794 73.47781 galactic CVn Second-epoch detections are separated by 3.9" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J210.4224+33.8268 | 14:01:41.82 +33:49:22.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J210.4224+33.8268,2461126.7770,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J210.4224+33.8268 20260327.2770 14.12CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:01:41.82 +33:49:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20_00sec_-10_00C_LIGHT_0267_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20_00sec_-10_00C_LIGHT_0266_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20_00sec_-10_00C_LIGHT_0267_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20_00sec_-10_00C_LIGHT_0266_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0431 Boo,2461126.7770,14.09,0.05,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
V0431 Boo 20260327.2770 14.09CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:05:26.50 +28:30:54.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20_00sec_-10_00C_LIGHT_0267_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20_00sec_-10_00C_LIGHT_0266_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20_00sec_-10_00C_LIGHT_0267_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20_00sec_-10_00C_LIGHT_0266_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0402 CVn,2461126.7770,12.76,0.05,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
V0402 CVn 20260327.2770 12.76CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:42:14.16 +28:25:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20_00sec_-10_00C_LIGHT_0267_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20_00sec_-10_00C_LIGHT_0266_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20_00sec_-10_00C_LIGHT_0267_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20_00sec_-15_00C_LIGHT_0364_fits__*pix.png resample_wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20_00sec_-10_00C_LIGHT_0266_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.89462175 22.02.2026 09:28:05.319 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
First image: 2461093.89462175 22.02.2026 09:28:05.319 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Last image: 2461126.77724176 27.03.2026 06:39:03.688 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5212
Objects passed selection criteria: 5203
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 4596.5
Average stars matched: 4498.75 (97.8734 %)
Memory usage VmPeak: 111844 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 01:42:28 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: 2461093.89462175 22.02.2026 09:28:05.319 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
First image: 2461093.89462175 22.02.2026 09:28:05.319 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Last image: 2461126.77724176 27.03.2026 06:39:03.688 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 41
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 9 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): 26484
Objects passed selection criteria: 26433
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 24213.5
Average stars matched: 23464.8 (96.9077 %)
Memory usage VmPeak: 130744 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 01:43:04 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat to cache
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.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/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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: 2461126.77671550
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits exists and is non-empty
Saving wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits to local_wcs_cache/
'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits' -> 'local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits'
wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits exists and is non-empty
Saving wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits to local_wcs_cache/
'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits' -> 'local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits'
wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits exists and is non-empty
Saving wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits to local_wcs_cache/
'wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits' -> 'local_wcs_cache/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits'
wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits exists and is non-empty
Saving wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits to local_wcs_cache/
'wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits' -> 'local_wcs_cache/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:00:01.192 +30:00:06.46
Second-epoch image center 13:59:55.886 +30:01:34.57
Angular distance between the image centers 0.03 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 14:00:01.192 +30:00:06.46
Second-epoch image center 13:59:57.228 +30:01:41.80
Angular distance between the image centers 0.03 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 13:59:55.886 +30:01:34.57
Second-epoch second image center 13:59:57.228 +30:01:41.80
Angular distance between the image centers 0.00524 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/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits &> /tmp/tmp.mjuwFPoZE5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits &> /tmp/tmp.pL6xWIbtDw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits &> /tmp/tmp.b0KB46LE6r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits &> /tmp/tmp.mNqvpBeZHP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.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_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits and wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.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_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits and wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
Found non-empty wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits and wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
The reference image (wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits) and catalog (wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat) found
'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3467 out of 6429 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.962862
a=0.000000 b=1.000000 c=22.962862
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
2.4 pix CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
2.4 pix fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
2.4 pix fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Limiting magnitude estimates:
15.4 mag. CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
15.5 mag. CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
15.0 mag. fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
15.0 mag. fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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.mjuwFPoZE5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits' -> 'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=335, passed=6429
Got 6429 stars (including 6086 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
util/solve_plate_with_UCAC5 got 6429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits -region wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.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.pL6xWIbtDw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits' -> 'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=363, passed=6415
Got 6415 stars (including 6043 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat
util/solve_plate_with_UCAC5 got 6415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits -region wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.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.b0KB46LE6r (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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
Checking if the catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
WCS catalog name: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=285, passed=4741
Got 4741 stars (including 4454 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 4741 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits -region wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.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.mNqvpBeZHP (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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Checking if the catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
WCS catalog name: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=288, passed=4729
Got 4729 stars (including 4439 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 4729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits -region wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits'
Saving fully-calibrated image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits'
Saving fully-calibrated image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits'
Saving fully-calibrated image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits'
Preparing the HTML report for the field CVn-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 20372_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 20372_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 13:35:03.78 +33:03:07.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field CVn-03-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 ####
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/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat to cache
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Creating symlink local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
Creating symlink local_wcs_cache/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
Creating symlink local_wcs_cache/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits exists and is non-empty
wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits exists and is non-empty
wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits exists and is non-empty
wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:00:01.192 +30:00:06.46
Second-epoch image center 13:59:55.886 +30:01:34.57
Angular distance between the image centers 0.03 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 14:00:01.192 +30:00:06.46
Second-epoch image center 13:59:57.228 +30:01:41.80
Angular distance between the image centers 0.03 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 13:59:55.886 +30:01:34.57
Second-epoch second image center 13:59:57.228 +30:01:41.80
Angular distance between the image centers 0.00524 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/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits &> /tmp/tmp.43m0UR9IVo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits &> /tmp/tmp.FlsRMgw03U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits &> /tmp/tmp.UO7X3mTNig
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits &> /tmp/tmp.NRTZSdxHYN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.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_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits and wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.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_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits and wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
Found non-empty wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits and wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
The reference image (wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits) and catalog (wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat) found
'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3484 out of 31021 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.843773
a=0.000000 b=1.000000 c=22.843773
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 27 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
2.2 pix CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
2.2 pix fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
2.2 pix fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Limiting magnitude estimates:
15.6 mag. CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
15.6 mag. CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
15.2 mag. fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
15.2 mag. fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.43m0UR9IVo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits' -> 'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1325, passed=31007
Got 31007 stars (including 29649 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat
util/solve_plate_with_UCAC5 got 31007 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits -region wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.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.FlsRMgw03U (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits' -> 'wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat corresponding to the image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1400, passed=31359
Got 31359 stars (including 29931 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat
util/solve_plate_with_UCAC5 got 31359 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits -region wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.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.UO7X3mTNig (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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
Checking if the catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
WCS catalog name: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=852, passed=24417
Got 24417 stars (including 23539 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat
util/solve_plate_with_UCAC5 got 24417 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits -region wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.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.NRTZSdxHYN (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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Checking if the catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat corresponding to the image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
WCS catalog name: wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=860, passed=24429
Got 24429 stars (including 23542 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat
util/solve_plate_with_UCAC5 got 24429 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits -region wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-05_20.00sec_-15.00C_LIGHT_0364.fits
Saving fully-calibrated image wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_CVn-03-Q2b1x1_2026-02-22_03-28-51_20.00sec_-15.00C_LIGHT_0365.fits
Saving fully-calibrated image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-38-18_20.00sec_-10.00C_LIGHT_0266.fits
Saving fully-calibrated image wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.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_2026-03-27_CI_CVn-03-Q2b1x1_014017_TTUQ2b1x1_19574_I0sR7Epe/wcs_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267.fits
Preparing the HTML report for the field CVn-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52254.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 2s
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Considering the candidate 52047_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52047_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 13:50:54.79 +28:34:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52048_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52048_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:11:45.13 +29:41:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 1.759 1453136286919051648 212.93747941215 +29.69331859569 14.9193 14.3614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52049_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52049_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:27:10.44 +33:05:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52052_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
Preparing report for the candidate 52052_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
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Considering the candidate 52053_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
Preparing report for the candidate 52053_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
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Considering the candidate 52057_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52057_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:27:36.12 +33:46:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52175_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52175_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 52191_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52191_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 52254_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
Preparing report for the candidate 52254_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
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Considering the candidate 52269_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52269_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 13:42:13.26 +28:19:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.174 1454781152022189568 205.55542794733 +28.33080555203 12.6356 11.8218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52275_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52275_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 13:31:07.42 +26:23:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52297_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52297_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 52300_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52300_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:11:14.35 +32:19:48.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52388_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52388_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 52408_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52408_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 52469_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52469_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:06:29.92 +27:42:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52506_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52506_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 52575_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52575_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 13:53:00.22 +28:05:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52585_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52585_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 52624_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52624_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 52639_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52639_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:01:04.75 +30:39:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52654_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52654_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:05:26.98 +28:33:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 5.285 1452629373406368128 211.36339401057 +28.55555199775 14.7567 14.0699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52681_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52681_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 52726_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52726_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 13:50:02.17 +29:15:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52768_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 52768_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:27:16.14 +30:18:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25698_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 25698_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks
**** FOUND 14:25:46.55 +32:37:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50034_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267
The candidate 50034_fd_CVn-03-Q2b1x1_2026-03-27_01-39-03_20.00sec_-10.00C_LIGHT_0267 did not pass the final checks