Mercurial > hg > octave-nkf
view scripts/plot/hist.m @ 14868:5d3a684236b0
maint: Use Octave coding conventions for cuddling parentheses in scripts directory
* lin2mu.m, loadaudio.m, wavread.m, accumarray.m, bicubic.m, celldisp.m,
colon.m, cplxpair.m, dblquad.m, divergence.m, genvarname.m, gradient.m,
int2str.m, interp1.m, interp1q.m, interp2.m, interpn.m, loadobj.m, nthargout.m,
__isequal__.m, __splinen__.m, quadgk.m, quadl.m, quadv.m, rat.m, rot90.m,
rotdim.m, saveobj.m, subsindex.m, triplequad.m, delaunay3.m, griddata.m,
inpolygon.m, tsearchn.m, voronoi.m, get_first_help_sentence.m, which.m,
gray2ind.m, pink.m, dlmwrite.m, strread.m, textread.m, textscan.m, housh.m,
ishermitian.m, issymmetric.m, krylov.m, logm.m, null.m, rref.m,
compare_versions.m, copyfile.m, dump_prefs.m, edit.m, fileparts.m,
getappdata.m, isappdata.m, movefile.m, orderfields.m, parseparams.m,
__xzip__.m, rmappdata.m, setappdata.m, swapbytes.m, unpack.m, ver.m, fminbnd.m,
fminunc.m, fsolve.m, glpk.m, lsqnonneg.m, qp.m, sqp.m, configure_make.m,
copy_files.m, describe.m, get_description.m, get_forge_pkg.m, install.m,
installed_packages.m, is_architecture_dependent.m, load_package_dirs.m,
print_package_description.m, rebuild.m, repackage.m, save_order.m, shell.m,
allchild.m, ancestor.m, area.m, axes.m, axis.m, clabel.m, close.m, colorbar.m,
comet.m, comet3.m, contour.m, cylinder.m, ezmesh.m, ezsurf.m, findobj.m,
fplot.m, hist.m, isocolors.m, isonormals.m, isosurface.m, isprop.m, legend.m,
mesh.m, meshz.m, pareto.m, pcolor.m, peaks.m, plot3.m, plotmatrix.m, plotyy.m,
polar.m, print.m, __add_datasource__.m, __add_default_menu__.m,
__axes_limits__.m, __bar__.m, __clabel__.m, __contour__.m, __errcomm__.m,
__errplot__.m, __ezplot__.m, __file_filter__.m, __fltk_print__.m,
__ghostscript__.m, __gnuplot_print__.m, __go_draw_axes__.m,
__go_draw_figure__.m, __interp_cube__.m, __marching_cube__.m, __patch__.m,
__pie__.m, __plt__.m, __print_parse_opts__.m, __quiver__.m, __scatter__.m,
__stem__.m, __tight_eps_bbox__.m, __uigetdir_fltk__.m, __uigetfile_fltk__.m,
__uiputfile_fltk__.m, quiver.m, quiver3.m, rectangle.m, refreshdata.m,
ribbon.m, scatter.m, semilogy.m, shading.m, slice.m, subplot.m, surface.m,
surfl.m, surfnorm.m, text.m, uigetfile.m, uiputfile.m, whitebg.m, deconv.m,
mkpp.m, pchip.m, polyaffine.m, polyder.m, polygcd.m, polyout.m, polyval.m,
ppint.m, ppjumps.m, ppval.m, residue.m, roots.m, spline.m, splinefit.m,
addpref.m, getpref.m, setpref.m, ismember.m, setxor.m, arch_fit.m, arch_rnd.m,
arch_test.m, autoreg_matrix.m, diffpara.m, fftconv.m, filter2.m, hanning.m,
hurst.m, periodogram.m, triangle_sw.m, sinc.m, spectral_xdf.m, spencer.m,
stft.m, synthesis.m, unwrap.m, yulewalker.m, bicgstab.m, gmres.m, pcg.m, pcr.m,
__sprand_impl__.m, speye.m, spfun.m, sprandn.m, spstats.m, svds.m,
treelayout.m, treeplot.m, bessel.m, factor.m, legendre.m, perms.m, primes.m,
magic.m, toeplitz.m, corr.m, cov.m, mean.m, median.m, mode.m, qqplot.m,
quantile.m, ranks.m, zscore.m, logistic_regression_likelihood.m,
bartlett_test.m, chisquare_test_homogeneity.m, chisquare_test_independence.m,
kolmogorov_smirnov_test.m, run_test.m, u_test.m, wilcoxon_test.m, z_test.m,
z_test_2.m, bin2dec.m, dec2base.m, mat2str.m, strcat.m, strchr.m, strjust.m,
strtok.m, substr.m, untabify.m, assert.m, demo.m, example.m, fail.m, speed.m,
test.m, now.m: Use Octave coding conventions for cuddling parentheses in
scripts directory.
author | Rik <octave@nomad.inbox5.com> |
---|---|
date | Tue, 17 Jul 2012 07:08:39 -0700 |
parents | e7c8e31f8e5d |
children | c2dbdeaa25df |
line wrap: on
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## Copyright (C) 1994-2012 John W. Eaton ## ## This file is part of Octave. ## ## Octave is free software; you can redistribute it and/or modify it ## under the terms of the GNU General Public License as published by ## the Free Software Foundation; either version 3 of the License, or (at ## your option) any later version. ## ## Octave is distributed in the hope that it will be useful, but ## WITHOUT ANY WARRANTY; without even the implied warranty of ## MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU ## General Public License for more details. ## ## You should have received a copy of the GNU General Public License ## along with Octave; see the file COPYING. If not, see ## <http://www.gnu.org/licenses/>. ## -*- texinfo -*- ## @deftypefn {Function File} {} hist (@var{y}) ## @deftypefnx {Function File} {} hist (@var{y}, @var{x}) ## @deftypefnx {Function File} {} hist (@var{y}, @var{nbins}) ## @deftypefnx {Function File} {} hist (@var{y}, @var{x}, @var{norm}) ## @deftypefnx {Function File} {[@var{nn}, @var{xx}] =} hist (@dots{}) ## @deftypefnx {Function File} {[@dots{}] =} hist (@dots{}, @var{prop}, @var{val}) ## ## Produce histogram counts or plots. ## ## With one vector input argument, @var{y}, plot a histogram of the values ## with 10 bins. The range of the histogram bins is determined by the ## range of the data. With one matrix input argument, @var{y}, plot a ## histogram where each bin contains a bar per input column. ## ## Given a second vector argument, @var{x}, use that as the centers of ## the bins, with the width of the bins determined from the adjacent ## values in the vector. ## ## If scalar, the second argument, @var{nbins}, defines the number of bins. ## ## If a third argument is provided, the histogram is normalized such that ## the sum of the bars is equal to @var{norm}. ## ## Extreme values are lumped in the first and last bins. ## ## With two output arguments, produce the values @var{nn} and @var{xx} such ## that @code{bar (@var{xx}, @var{nn})} will plot the histogram. ## ## The histogram's appearance may be modified by specifying property/value ## pairs, @var{prop} and @var{val} pairs. For example the face and edge ## color may be modified. ## ## @example ## @group ## hist (randn (1, 100), 25, "facecolor", "r", "edgecolor", "b"); ## @end group ## @end example ## ## @noindent ## The histograms colors also depend upon the colormap. ## ## @example ## @group ## hist (rand (10, 3)); ## colormap (summer ()); ## @end group ## @end example ## ## @seealso{bar} ## @end deftypefn ## Author: jwe function [nn, xx] = hist (y, varargin) if (nargin < 1) print_usage (); endif arg_is_vector = isvector (y); if (rows (y) == 1) y = y(:); endif if (isreal (y)) max_val = max (y(:)); min_val = min (y(:)); else error ("hist: first argument must be real valued"); endif iarg = 1; if (nargin == 1 || ischar (varargin{iarg})) n = 10; x = [0.5:n]'/n; x = x * (max_val - min_val) + ones (size (x)) * min_val; else ## nargin is either 2 or 3 x = varargin{iarg++}; if (isscalar (x)) n = x; if (n <= 0) error ("hist: number of bins must be positive"); endif x = [0.5:n]'/n; x = x * (max_val - min_val) + ones (size (x)) * min_val; elseif (isreal (x)) if (isvector (x)) x = x(:); endif tmp = sort (x); if (any (tmp != x)) warning ("hist: bin values not sorted on input"); x = tmp; endif else error ("hist: second argument must be a scalar or a vector"); endif endif ## Avoid issues with integer types for x and y x = double (x); y = double (y); cutoff = (x(1:end-1,:) + x(2:end,:)) / 2; n = rows (x); y_nc = columns (y); if (n < 30 && columns (x) == 1) ## The following algorithm works fastest for n less than about 30. chist = zeros (n+1, y_nc); for i = 1:n-1 chist(i+1,:) = sum (y <= cutoff(i)); endfor chist(n+1,:) = sum (! isnan (y)); else ## The following algorithm works fastest for n greater than about 30. ## Put cutoff elements between boundaries, integrate over all ## elements, keep totals at boundaries. [s, idx] = sort ([y; repmat(cutoff, 1, y_nc)]); len = rows (y); chist = cumsum (idx <= len); chist = [(zeros (1, y_nc)); (reshape (chist(idx > len), rows (cutoff), y_nc)); (chist(end,:) - sum (isnan (y)))]; endif freq = diff (chist); if (nargin > 2 && ! ischar (varargin{iarg})) ## Normalise the histogram. norm = varargin{iarg++}; freq = freq / sum(! isnan (y)) * norm; endif if (nargout > 0) if (arg_is_vector) nn = freq'; xx = x'; else nn = freq; xx = x; endif elseif (size (freq, 2) != 1) bar (x, freq, 0.8, varargin{iarg:end}); else bar (x, freq, 1.0, varargin{iarg:end}); endif endfunction %!test %! [nn,xx] = hist ([1:4], 3); %! assert (xx, [1.5,2.5,3.5]); %! assert (nn, [2,1,1]); %!test %! [nn,xx] = hist ([1:4]', 3); %! assert (xx, [1.5,2.5,3.5]); %! assert (nn, [2,1,1]); %!test %! [nn,xx] = hist ([1 1 1 NaN NaN NaN 2 2 3],[1 2 3]); %! assert (xx, [1,2,3]); %! assert (nn, [3,2,1]); %!test %! [nn,xx] = hist ([1 1 1 NaN NaN NaN 2 2 3],[1 2 3], 6); %! assert (xx, [1,2,3]); %! assert (nn, [3,2,1]); %!test %! [nn,xx] = hist ([[1:4]', [1:4]'], 3); %! assert (xx, [1.5;2.5;3.5]); %! assert (nn, [[2,1,1]',[2,1,1]']); %!test %! for n = [10, 30, 100, 1000] %! assert (sum (hist ([1:n], n)), n); %! assert (sum (hist ([1:n], [2:n-1])), n); %! assert (sum (hist ([1:n], [1:n])), n); %! assert (sum (hist ([1:n], 29)), n); %! assert (sum (hist ([1:n], 30)), n); %! endfor %!assert (hist (1,1), 1) %!assert (size (hist (randn (750,240), 200)), [200,240])