NAME

       NoiseChisel - detect signal in a noisy image

SYNOPSIS

       astnoisechisel [OPTION...] ASTRdata

DESCRIPTION

       NoiseChisel  is  part  of  GNU  Astronomy Utilities 0.5.  NoiseChisel Detects and segments signal that is
       deeply burried in noise. It employs a noise-based detection and segmentation method  enabling  it  to  be
       very resilient to the rich diversity of shapes in astronomical targets.

       For  more information, please run any of the following commands. In particular the second contains a very
       comprehensive  explanation  of  NoiseChisel's  invocation:  expected  input(s),  output(s),  and  a  full
       description of all the options.

       All options and their values:
              $ astnoisechisel -P

       Inputs/Outputs and options:
              $ info astnoisechisel

       Full section in manual/book:
              $ info NoiseChisel

       Full Gnuastro manual/book:
              $ info gnuastro

       If  you  couldn't find your answer in the manual, you can get direct help from experienced Gnuastro users
       and developers. For more information, please run:

              $ info help-gnuastro

       NoiseChisel options:

              Input:

       -B, --minskyfrac=FLT
              Min. fraction of undetected area in tile.

       --convolved=STR
              Convolved image file to avoid convolution.

       --convolvedhdu=STR
              HDU/extension of convolved image in file.

       -E, --skysubtracted
              Input is Sky subtracted (for error estimation).

       -h, --hdu=STR/INT
              Extension name or number of input data.

       -k, --kernel=STR
              Filename of kernel to convolve with input

       --khdu=STR
              HDU containing kernel image.

       --minnumfalse=INT
              Minimum number for S/N estimation.

       -w, --widekernel=STR
              Filename of wider kernel for better qthresh

       --wkhdu=STR
              HDU containing wide kernel image.

              Tessellation (tile grid):

       --checktiles
              Tile IDs in an image, the size of input.

       -F, --remainderfrac=FLT
              Fraction of remainder to split last tile.

       --interpnumngb=INT
              No. of neighbors to use for interpolation.

       --interponlyblank
              Only interpolate over the blank tiles.

       -L, --largetilesize=INT[,INT]
              Sim. to --tilesize, but for larger tiles.

       -M, --numchannels=INT[,..] No. of channels in dim.s (FITS order).

       --oneelempertile
              Display 1 element/tile, not full input res.

       --workoverch
              Work (not tile) over channel edges.

       -Z, --tilesize=INT[,INT]
              Regular tile size on dim.s (FITS order).

              Output:

       -D, --dontdelete
              Don't delete output if it exists.

       -K, --keepinputdir
              Keep input directory for automatic output.

       --onlydetection
              Stop at the end of detection.

       -o, --output=STR
              Output name.

       --tableformat=STR
              `txt', `fits-ascii', `fits-binary'.

              Detection:

       --checkdetection
              Save all the detection steps to a file.

       --checkdetsky
              Save Sky value estimation for pseudo-dets.

       --checkdetsn
              Save pseudo-detection S/N values to a file.

       --checkqthresh
              Save quantile threshold estimation in file.

       -c, --detquant=FLT
              Quantile in pseudo-det. to define true.

       --checksky
              Final sky and its STD steps in a file.

       --cleangrowndet
              Remove small S/N grown detections.

       -d, --detgrowquant=FLT
              Minimum quant. to expand true detections.

       --detgrowmaxholesize=INT
              Max. area of holes after growth to fill.

       -e, --erode=INT
              Number of erosions after thresholding.

       --erodengb=INT
              4 or 8 connectivity in erosion.

       -i, --detsnminarea=INT
              Min. pseudo-detection area for S/N dist.

       --noerodequant=FLT
              Quantile for no erosion.

       --openingngb=INT
              4 or 8 connectivity in opening.

       -p, --opening=INT
              Depth of opening after erosion.

       --qthreshtilequant=FLT Remove tiles at higher quantiles.

       -Q, --modmedqdiff=FLT
              Max. mode and median quant diff. per tile.

       -r, --mirrordist=FLT
              Max. dist. (error multip.) to find mode.

       -R, --dthresh=FLT
              Sigma threshold for Pseudo-detections.

       --smoothwidth=INT
              Flat kernel width to smooth interpolated.

       -s, --sigmaclip=FLT,FLT
              Sigma multiple and, tolerance or number.

       -t, --qthresh=FLT
              Quantile threshold on convolved image.

              Segmentation:

       --checkclumpsn
              Save Sky clump S/N values into a file.

       --checksegmentation
              Store segmentation steps in a file.

       -g, --segquant=FLT
              S/N Quantile of true sky clumps.

       --grownclumps
              Save grown clumps instead of original.

       -G, --gthresh=FLT
              Multiple of STD to stop growing clumps.

       -m, --segsnminarea=INT
              Minimum area of clumps for S/N estimation.

       -O, --objbordersn=FLT
              Min. S/N for grown clumps as one object.

       -v, --keepmaxnearriver
              Keep clumps with peak touching a river.

       -y, --minriverlength=INT
              Minimum len of useful grown clump rivers.

              Operating modes:

       -?, --help
              give this help list

       --cite BibTeX citation for this program.

       --config=STR
              Read configuration file STR immediately.

       -C, --continueaftercheck
              Continue processing after checks.

       --lastconfig
              Do not parse any more configuration files.

       --minmapsize=INT
              Minimum bytes in array to not use ram RAM.

       -N, --numthreads=INT
              Number of CPU threads to use.

       --onlyversion=STR
              Only run if the program version is STR.

       -P, --printparams
              Print parameter values to be used and abort.

       -q, --quiet
              Only report errors, remain quiet about steps.

       -S, --setdirconf
              Set default values for this directory and abort.

       --usage
              give a short usage message

       -U, --setusrconf
              Set default values for this user and abort.

       -V, --version
              print program version

       Mandatory or optional arguments to long options are also mandatory  or  optional  for  any  corresponding
       short options.

       GNU Astronomy Utilities home page: http://www.gnu.org/software/gnuastro/

REPORTING BUGS

       Report bugs to bug-gnuastro@gnu.org.

COPYRIGHT

       Copyright © 2015-2017, Free Software Foundation, Inc.  License GPLv3+: GNU General public license version
       3 or later.
       This  is  free software: you are free to change and redistribute it.  There is NO WARRANTY, to the extent
       permitted by law.

       Written/developed by Mohammad Akhlaghi

SEE ALSO

       The full documentation for NoiseChisel is maintained as a Texinfo manual.  If the  info  and  NoiseChisel
       programs are properly installed at your site, the command

              info NoiseChisel

       should give you access to the complete manual.

GNU Astronomy Utilities 0.5                       December 2017                                   NOISECHISEL(1)