Mercurial > octave
changeset 21546:f7f97d7e9294
doc: Wrap m-file docstrings to 79 characters + newline (80 total).
* isrecording.m, soundsc.m, delaunay3.m, cell2mat.m, cumtrapz.m, del2.m,
inputParser.m, interp1.m, interp3.m, narginchk.m, profile.m,
validateattributes.m, delaunayn.m, tsearchn.m, voronoin.m, brighten.m,
cmunique.m, colorcube.m, imfinfo.m, imshow.m, edit.m, orderfields.m, run.m,
warning_ids.m, ode23.m, ode45.m, odeget.m, integrate_adaptive.m, kahan.m,
ode_struct_value_check.m, runge_kutta_23.m, fminunc.m, fsolve.m, fzero.m,
pkg.m, build.m, specular.m, view.m, bar.m, barh.m, contour3.m, isosurface.m,
line.m, pie.m, pie3.m, quiver3.m, scatter.m, scatter3.m, stem3.m, stemleaf.m,
surfl.m, tetramesh.m, isfigure.m, mkpp.m, pchip.m, residue.m, splinefit.m,
rmpref.m, unique.m, eigs.m, ilu.m, factor.m, factorial.m, gallery.m, hankel.m,
histc.m, ols.m, finv.m, fpdf.m, kruskal_wallis_test.m, weekday.m:
Wrap m-file docstrings to 79 characters + newline (80 total).
line wrap: on
line diff
--- a/scripts/audio/@audiorecorder/isrecording.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/audio/@audiorecorder/isrecording.m Sun Mar 27 15:50:01 2016 -0700 @@ -18,8 +18,8 @@ ## -*- texinfo -*- ## @deftypefn {} {} isrecording (@var{recorder}) -## Return true if the audiorecorder object @var{recorder} is currently recording -## audio and false otherwise. +## Return true if the audiorecorder object @var{recorder} is currently +## recording audio and false otherwise. ## @end deftypefn function result = isrecording (recorder)
--- a/scripts/audio/soundsc.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/audio/soundsc.m Sun Mar 27 15:50:01 2016 -0700 @@ -33,10 +33,10 @@ ## The optional argument @var{nbits} specifies the bit depth to play to the ## audio device and defaults to 8 bits. ## -## By default, @var{y} is automatically normalized to the range [-1, 1]. If the -## range [@var{ymin}, @var{ymax}] is given, then elements of @var{y} that fall -## within the range @var{ymin} @leq{} @var{y} @leq{} @var{ymax} are scaled to -## the range [-1, 1] instead. +## By default, @var{y} is automatically normalized to the range [-1, 1]. If +## the range [@var{ymin}, @var{ymax}] is given, then elements of @var{y} +## that fall within the range @var{ymin} @leq{} @var{y} @leq{} @var{ymax} +## are scaled to the range [-1, 1] instead. ## ## For more control over audio playback, use the @code{audioplayer} class. ## @seealso{sound, record}
--- a/scripts/deprecated/delaunay3.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/deprecated/delaunay3.m Sun Mar 27 15:50:01 2016 -0700 @@ -35,9 +35,9 @@ ## @var{x}, @var{y}, @var{z} for the location of the j-th vertex of the i-th ## tetrahedron. ## -## An optional fourth argument, which must be a string or cell array of strings, -## contains options passed to the underlying qhull command. -## See the documentation for the Qhull library for details +## An optional fourth argument, which must be a string or cell array of +## strings, contains options passed to the underlying qhull command. See the +## documentation for the Qhull library for details ## @url{http://www.qhull.org/html/qh-quick.htm#options}. ## The default options are @code{@{"Qt", "Qbb", "Qc", "Qz"@}}. ##
--- a/scripts/general/cell2mat.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/cell2mat.m Sun Mar 27 15:50:01 2016 -0700 @@ -23,7 +23,8 @@ ## elements of @var{c} into a hyperrectangle. ## ## Elements of @var{c} must be numeric, logical, or char matrices; or cell -## arrays; or structs; and @code{cat} must be able to concatenate them together. +## arrays; or structs; and @code{cat} must be able to concatenate them +## together. ## @seealso{mat2cell, num2cell} ## @end deftypefn
--- a/scripts/general/cumtrapz.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/cumtrapz.m Sun Mar 27 15:50:01 2016 -0700 @@ -31,7 +31,8 @@ ## When the argument @var{x} is omitted an equally spaced @var{x} vector with ## unit spacing (1) is assumed. @code{cumtrapz (@var{x}, @var{y})} evaluates ## the integral with respect to the spacing in @var{x} and the values in -## @var{y}. This is useful if the points in @var{y} have been sampled unevenly. +## @var{y}. This is useful if the points in @var{y} have been sampled +## unevenly. ## ## If the optional @var{dim} argument is given, operate along this dimension. ##
--- a/scripts/general/del2.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/del2.m Sun Mar 27 15:50:01 2016 -0700 @@ -45,8 +45,8 @@ ## @end example ## ## @end ifnottex -## For N-dimensional arrays the sum in parentheses is expanded to include second -## derivatives over the additional higher dimensions. +## For N-dimensional arrays the sum in parentheses is expanded to include +## second derivatives over the additional higher dimensions. ## ## The spacing between evaluation points may be defined by @var{h}, which is a ## scalar defining the equidistant spacing in all dimensions. Alternatively,
--- a/scripts/general/inputParser.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/inputParser.m Sun Mar 27 15:50:01 2016 -0700 @@ -148,8 +148,8 @@ ## -*- texinfo -*- ## @deftypefn {} {} addOptional (@var{argname}, @var{default}) ## @deftypefnx {} {} addOptional (@var{argname}, @var{default}, @var{validator}) -## Add new optional argument to the object @var{parser} of the class inputParser -## to implement an ordered arguments type of API +## Add new optional argument to the object @var{parser} of the class +## inputParser to implement an ordered arguments type of API ## ## @var{argname} must be a string with the name of the new argument. The order ## in which new arguments are added with @command{addOptional}, represents the
--- a/scripts/general/interp1.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/interp1.m Sun Mar 27 15:50:01 2016 -0700 @@ -75,8 +75,8 @@ ## be supplied and @code{interp1} returns a piecewise polynomial object. This ## object can later be used with @code{ppval} to evaluate the interpolation. ## There is an equivalence, such that @code{ppval (interp1 (@var{x}, -## @var{y}, @var{method}, @qcode{"pp"}), @var{xi}) == interp1 (@var{x}, @var{y}, -## @var{xi}, @var{method}, @qcode{"extrap"})}. +## @var{y}, @var{method}, @qcode{"pp"}), @var{xi}) == interp1 (@var{x}, +## @var{y}, @var{xi}, @var{method}, @qcode{"extrap"})}. ## ## Duplicate points in @var{x} specify a discontinuous interpolant. There ## may be at most 2 consecutive points with the same value.
--- a/scripts/general/interp3.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/interp3.m Sun Mar 27 15:50:01 2016 -0700 @@ -44,12 +44,12 @@ ## not important. ## ## If called with a single reference data matrix @var{v} and a refinement -## value @var{n}, then perform interpolation over a 3-D grid where each original -## interval has been recursively subdivided @var{n} times. This results in -## @code{2^@var{n}-1} additional points for every interval in the original -## grid. If @var{n} is omitted a value of 1 is used. As an example, the -## interval [0,1] with @code{@var{n}==2} results in a refined interval with -## points at [0, 1/4, 1/2, 3/4, 1]. +## value @var{n}, then perform interpolation over a 3-D grid where each +## original interval has been recursively subdivided @var{n} times. This +## results in @code{2^@var{n}-1} additional points for every interval in the +## original grid. If @var{n} is omitted a value of 1 is used. As an +## example, the interval [0,1] with @code{@var{n}==2} results in a refined +## interval with points at [0, 1/4, 1/2, 3/4, 1]. ## ## The interpolation @var{method} is one of: ##
--- a/scripts/general/narginchk.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/narginchk.m Sun Mar 27 15:50:01 2016 -0700 @@ -21,11 +21,12 @@ ## Check for correct number of input arguments. ## ## Generate an error message if the number of arguments in the calling function -## is outside the range @var{minargs} and @var{maxargs}. Otherwise, do nothing. +## is outside the range @var{minargs} and @var{maxargs}. Otherwise, do +## nothing. ## ## Both @var{minargs} and @var{maxargs} must be scalar numeric values. Zero, -## Inf, and negative values are all allowed, and @var{minargs} and @var{maxargs} -## may be equal. +## Inf, and negative values are all allowed, and @var{minargs} and +## @var{maxargs} may be equal. ## ## Note that this function evaluates @code{nargin} on the caller. ##
--- a/scripts/general/profile.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/profile.m Sun Mar 27 15:50:01 2016 -0700 @@ -41,9 +41,9 @@ ## statistics are added to the existing ones. ## ## @item @var{S} = profile ("status") -## Return a structure with information about the current status of the profiler. -## At the moment, the only field is @code{ProfilerStatus} which is either -## @qcode{"on"} or @qcode{"off"}. +## Return a structure with information about the current status of the +## profiler. At the moment, the only field is @code{ProfilerStatus} which is +## either @qcode{"on"} or @qcode{"off"}. ## ## @item @var{T} = profile ("info") ## Return the collected profiling statistics in the structure @var{T}. The
--- a/scripts/general/validateattributes.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/general/validateattributes.m Sun Mar 27 15:50:01 2016 -0700 @@ -55,7 +55,8 @@ ## ## @table @asis ## @item @qcode{"<="} -## All values are less than or equal to the following value in @var{attributes}. +## All values are less than or equal to the following value in +## @var{attributes}. ## ## @item @qcode{"<"} ## All values are less than the following value in @var{attributes}.
--- a/scripts/geometry/delaunayn.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/geometry/delaunayn.m Sun Mar 27 15:50:01 2016 -0700 @@ -31,9 +31,9 @@ ## @var{pts} which describes a simplex of dimension dim. For example, a 2-D ## simplex is a triangle and 3-D simplex is a tetrahedron. ## -## An optional second argument, which must be a string or cell array of strings, -## contains options passed to the underlying qhull command. -## See the documentation for the Qhull library for details +## An optional second argument, which must be a string or cell array of +## strings, contains options passed to the underlying qhull command. See the +## documentation for the Qhull library for details ## @url{http://www.qhull.org/html/qh-quick.htm#options}. ## The default options depend on the dimension of the input: ##
--- a/scripts/geometry/tsearchn.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/geometry/tsearchn.m Sun Mar 27 15:50:01 2016 -0700 @@ -25,8 +25,8 @@ ## containing the points @var{xi}. For points outside the convex hull, ## @var{idx} is NaN. ## -## If requested @code{tsearchn} also returns the Barycentric coordinates @var{p} -## of the enclosing triangles. +## If requested @code{tsearchn} also returns the Barycentric coordinates +## @var{p} of the enclosing triangles. ## @seealso{delaunay, delaunayn} ## @end deftypefn
--- a/scripts/geometry/voronoin.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/geometry/voronoin.m Sun Mar 27 15:50:01 2016 -0700 @@ -27,9 +27,9 @@ ## @var{C} contains the points of the Voronoi facets. The list @var{F} ## contains, for each facet, the indices of the Voronoi points. ## -## An optional second argument, which must be a string or cell array of strings, -## contains options passed to the underlying qhull command. -## See the documentation for the Qhull library for details +## An optional second argument, which must be a string or cell array of +## strings, contains options passed to the underlying qhull command. See the +## documentation for the Qhull library for details ## @url{http://www.qhull.org/html/qh-quick.htm#options}. ## ## The default options depend on the dimension of the input:
--- a/scripts/image/brighten.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/image/brighten.m Sun Mar 27 15:50:01 2016 -0700 @@ -32,7 +32,8 @@ ## The first argument can also be a valid graphics handle @var{h}, in which ## case @code{brighten} is applied to the colormap associated with this handle. ## -## If no output is specified then the result is written to the current colormap. +## If no output is specified then the result is written to the current +## colormap. ## @seealso{colormap, contrast} ## @end deftypefn
--- a/scripts/image/cmunique.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/image/cmunique.m Sun Mar 27 15:50:01 2016 -0700 @@ -30,9 +30,9 @@ ## the indices adjusted to match the new, possibly smaller, colormap. ## ## When the input is an RGB image (an @nospell{MxNx3} array), the output -## colormap will contain one entry for every unique color in the original image. -## In the worst case the new map could have as many rows as the number of -## pixels in the original image. +## colormap will contain one entry for every unique color in the original +## image. In the worst case the new map could have as many rows as the +## number of pixels in the original image. ## ## When the input is a grayscale image @var{I}, the output colormap will ## contain one entry for every unique intensity value in the original image.
--- a/scripts/image/colorcube.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/image/colorcube.m Sun Mar 27 15:50:01 2016 -0700 @@ -22,9 +22,9 @@ ## Create color colormap. This colormap is composed of as many equally ## spaced colors (not grays) in the RGB color space as possible. ## -## If there are not a perfect number @var{n} of regularly spaced colors then the -## remaining entries in the colormap are gradients of pure red, green, blue, -## and gray. +## If there are not a perfect number @var{n} of regularly spaced colors then +## the remaining entries in the colormap are gradients of pure red, green, +## blue, and gray. ## ## The argument @var{n} must be a scalar. ## If unspecified, the length of the current colormap, or 64, is used.
--- a/scripts/image/imfinfo.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/image/imfinfo.m Sun Mar 27 15:50:01 2016 -0700 @@ -73,8 +73,8 @@ ## Number of iterations to loop an animation. ## ## @item ByteOrder -## Endian option for formats that support it. Value is @qcode{"little-endian"}, -## @qcode{"big-endian"}, or @qcode{"undefined"}. +## Endian option for formats that support it. Value is +## @qcode{"little-endian"}, @qcode{"big-endian"}, or @qcode{"undefined"}. ## ## @item Gamma ## Gamma level of the image. The same color image displayed on two different
--- a/scripts/image/imshow.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/image/imshow.m Sun Mar 27 15:50:01 2016 -0700 @@ -50,12 +50,14 @@ ## @item @qcode{"xdata"} ## If @var{value1} is a two element vector, it must contain horizontal axis ## limits in the form [xmin xmax]; Otherwise @var{value1} must be a vector and -## only the first and last elements will be used for xmin and xmax respectively. +## only the first and last elements will be used for xmin and xmax +## respectively. ## ## @item @qcode{"ydata"} ## If @var{value1} is a two element vector, it must contain vertical axis ## limits in the form [ymin ymax]; Otherwise @var{value1} must be a vector and -## only the first and last elements will be used for ymin and ymax respectively. +## only the first and last elements will be used for ymin and ymax +## respectively. ## ## @end table ##
--- a/scripts/miscellaneous/edit.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/miscellaneous/edit.m Sun Mar 27 15:50:01 2016 -0700 @@ -44,9 +44,9 @@ ## @item ## If @code{@var{name}.cc} is specified, then it will search for ## @code{@var{name}.cc} in the path and try to modify it, otherwise it will -## create a new @file{.cc} file in the current directory. If @var{name} happens -## to be an m-file or interpreter defined function, then the text of that -## function will be inserted into the .cc file as a comment. +## create a new @file{.cc} file in the current directory. If @var{name} +## happens to be an m-file or interpreter defined function, then the text of +## that function will be inserted into the .cc file as a comment. ## ## @item ## If @file{@var{name}.ext} is on your path then it will be edited, otherwise @@ -63,11 +63,11 @@ ## If @code{edit} is called with @var{field} and @var{value} variables, the ## value of the control field @var{field} will be set to @var{value}. ## -## If an output argument is requested and the first input argument is @code{get} -## then @code{edit} will return the value of the control field @var{field}. -## If the control field does not exist, edit will return a structure -## containing all fields and values. Thus, @code{edit ("get", "all")} returns -## a complete control structure. +## If an output argument is requested and the first input argument is +## @code{get} then @code{edit} will return the value of the control field +## @var{field}. If the control field does not exist, edit will return a +## structure containing all fields and values. Thus, @code{edit ("get", +## "all")} returns a complete control structure. ## ## The following control fields are used: ##
--- a/scripts/miscellaneous/orderfields.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/miscellaneous/orderfields.m Sun Mar 27 15:50:01 2016 -0700 @@ -27,10 +27,10 @@ ## ## Given one input struct @var{s1}, arrange field names alphabetically. ## -## If a second struct argument is given, arrange field names in @var{s1} as they -## appear in @var{s2}. The second argument may also specify the order in a -## cell array of strings @var{cellstr}. The second argument may also be a -## permutation vector. +## If a second struct argument is given, arrange field names in @var{s1} as +## they appear in @var{s2}. The second argument may also specify the order +## in a cell array of strings @var{cellstr}. The second argument may also +## be a permutation vector. ## ## The optional second output argument @var{p} is the permutation vector which ## converts the original name order to the new name order.
--- a/scripts/miscellaneous/run.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/miscellaneous/run.m Sun Mar 27 15:50:01 2016 -0700 @@ -26,9 +26,9 @@ ## their name. For scripts not located on the load path, use @code{run}. ## ## The filename @var{script} can be a bare, fully qualified, or relative -## filename and with or without a file extension. If no extension is specified, -## Octave will first search for a script with the @file{".m"} extension before -## falling back to the script name without an extension. +## filename and with or without a file extension. If no extension is +## specified, Octave will first search for a script with the @file{".m"} +## extension before falling back to the script name without an extension. ## ## Implementation Note: If @var{script} includes a path component, then ## @code{run} first changes the working directory to the directory where
--- a/scripts/miscellaneous/warning_ids.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/miscellaneous/warning_ids.m Sun Mar 27 15:50:01 2016 -0700 @@ -120,7 +120,8 @@ ## paths to function files. This usually happens when using autoload() ## calls in PKG_ADD files, when the PKG_ADD file is not in the same ## directory as the .oct file referred to by the autoload() command. -## By default, the @code{Octave:autoload-relative-file-name} warning is enabled. +## By default, the @code{Octave:autoload-relative-file-name} warning is +## enabled. ## ## @item Octave:built-in-variable-assignment ## By default, the @code{Octave:built-in-variable-assignment} warning is
--- a/scripts/ode/ode23.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/ode/ode23.m Sun Mar 27 15:50:01 2016 -0700 @@ -65,8 +65,8 @@ ## The output can also be returned as a structure @var{solution} which ## has field @var{x} containing the time where the solution was evaluated and ## field @var{y} containing the solution matrix for the times in @var{x}. -## Use @code{fieldnames (@var{solution})} to see the other fields and additional -## information returned. +## Use @code{fieldnames (@var{solution})} to see the other fields and +## additional information returned. ## ## If using the @qcode{"Events"} option then three additional outputs may ## be returned. @var{te} holds the time when an Event function returned a @@ -76,10 +76,10 @@ ## ## This function can be called with two output arguments: @var{t} and @var{y}. ## Variable @var{t} is a column vector and contains the time stamps, instead -## @var{y} is a matrix in which each column refers to a different unknown of the -## problem and the rows number is the same of @var{t} rows number so that each -## row of @var{y} contains the values of all unknowns at the time value -## contained in the corresponding row in @var{t}. +## @var{y} is a matrix in which each column refers to a different unknown of +## the problem and the rows number is the same of @var{t} rows number so +## that each row of @var{y} contains the values of all unknowns at the time +## value contained in the corresponding row in @var{t}. ## ## Example: Solve the @nospell{Van der Pol} equation ##
--- a/scripts/ode/ode45.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/ode/ode45.m Sun Mar 27 15:50:01 2016 -0700 @@ -63,8 +63,8 @@ ## The output can also be returned as a structure @var{solution} which ## has field @var{x} containing the time where the solution was evaluated and ## field @var{y} containing the solution matrix for the times in @var{x}. -## Use @code{fieldnames (@var{solution})} to see the other fields and additional -## information returned. +## Use @code{fieldnames (@var{solution})} to see the other fields and +## additional information returned. ## ## If using the @qcode{"Events"} option then three additional outputs may ## be returned. @var{te} holds the time when an Event function returned a
--- a/scripts/ode/odeget.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/ode/odeget.m Sun Mar 27 15:50:01 2016 -0700 @@ -24,10 +24,10 @@ ## Query the value of the property @var{field} in the ODE options structure ## @var{ode_opt}. ## -## If called with two input arguments and the first input argument @var{ode_opt} -## is an ODE option structure and the second input argument @var{field} is a -## string specifying an option name, then return the option value @var{val} -## corresponding to @var{field} from @var{ode_opt}. +## If called with two input arguments and the first input argument +## @var{ode_opt} is an ODE option structure and the second input argument +## @var{field} is a string specifying an option name, then return the option +## value @var{val} corresponding to @var{field} from @var{ode_opt}. ## ## If called with an optional third input argument, and @var{field} is ## not set in the structure @var{ode_opt}, then return the default value
--- a/scripts/ode/private/integrate_adaptive.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/ode/private/integrate_adaptive.m Sun Mar 27 15:50:01 2016 -0700 @@ -55,7 +55,8 @@ ## are taken as times at which the solution is required. ## ## The fifth argument represents the initial conditions for the ODEs and the -## last input argument contains some options that may be needed for the stepper. +## last input argument contains some options that may be needed for the +## stepper. ## ## @end deftypefn ##
--- a/scripts/ode/private/kahan.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/ode/private/kahan.m Sun Mar 27 15:50:01 2016 -0700 @@ -38,7 +38,8 @@ ## as the second output argument so that it can be reused in future calls of ## the same summation. ## -## The third input argument @var{term} is the variable to be added to @var{sum}. +## The third input argument @var{term} is the variable to be added to +## @var{sum}. ## @end deftypefn function [sum, comp] = kahan (sum, comp, term)
--- a/scripts/ode/private/ode_struct_value_check.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/ode/private/ode_struct_value_check.m Sun Mar 27 15:50:01 2016 -0700 @@ -22,7 +22,8 @@ ## @deftypefnx {} {} ode_struct_value_check (@var{"caller"), @var{ode_struct}, @var{"solver"}) ## @deftypefnx {} {@var{ode_struct} =} ode_struct_value_check (@dots{}) ## -## Validate the fields and values in the ODE options structure @var{ode_struct}. +## Validate the fields and values in the ODE options structure +## @var{ode_struct}. ## ## The first argument @var{caller} is a string with the name of the calling ## function so that warning and error messages properly display the source
--- a/scripts/ode/private/runge_kutta_23.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/ode/private/runge_kutta_23.m Sun Mar 27 15:50:01 2016 -0700 @@ -31,8 +31,8 @@ ## @url{http://en.wikipedia.org/wiki/List_of_Runge%E2%80%93Kutta_methods}. ## ## @var{@fun} is a function handle that defines the ODE: @code{y' = f(tau,y)}. -## The function must accept two inputs where the first is time @var{tau} and the -## second is a column vector of unknowns @var{y}. +## The function must accept two inputs where the first is time @var{tau} and +## the second is a column vector of unknowns @var{y}. ## ## @var{t} is the first extreme of integration interval. ##
--- a/scripts/optimization/fminunc.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/optimization/fminunc.m Sun Mar 27 15:50:01 2016 -0700 @@ -41,11 +41,11 @@ ## @qcode{"AutoScaling"}. ## ## If @qcode{"GradObj"} is @qcode{"on"}, it specifies that @var{fcn}, when -## called with two output arguments, also returns the Jacobian matrix of partial -## first derivatives at the requested point. @code{TolX} specifies the -## termination tolerance for the unknown variables @var{x}, while @code{TolFun} -## is a tolerance for the objective function value @var{fval}. The default is -## @code{1e-7} for both options. +## called with two output arguments, also returns the Jacobian matrix of +## partial first derivatives at the requested point. @code{TolX} specifies +## the termination tolerance for the unknown variables @var{x}, while +## @code{TolFun} is a tolerance for the objective function value @var{fval}. +## The default is @code{1e-7} for both options. ## ## For a description of the other options, see @code{optimset}. ## @@ -76,9 +76,10 @@ ## The trust region radius became excessively small. ## @end table ## -## Optionally, @code{fminunc} can return a structure with convergence statistics -## (@var{output}), the output gradient (@var{grad}) at the solution @var{x}, -## and approximate Hessian (@var{hess}) at the solution @var{x}. +## Optionally, @code{fminunc} can return a structure with convergence +## statistics (@var{output}), the output gradient (@var{grad}) at the +## solution @var{x}, and approximate Hessian (@var{hess}) at the solution +## @var{x}. ## ## Application Notes: If the objective function is a single nonlinear equation ## of one variable then using @code{fminbnd} is usually a better choice.
--- a/scripts/optimization/fsolve.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/optimization/fsolve.m Sun Mar 27 15:50:01 2016 -0700 @@ -53,9 +53,9 @@ ## ## If @qcode{"Updating"} is @qcode{"on"}, the function will attempt to use ## @nospell{Broyden} updates to update the Jacobian, in order to reduce the -## amount of Jacobian calculations. If your user function always calculates the -## Jacobian (regardless of number of output arguments) then this option provides -## no advantage and should be set to false. +## amount of Jacobian calculations. If your user function always calculates +## the Jacobian (regardless of number of output arguments) then this option +## provides no advantage and should be set to false. ## ## @qcode{"ComplexEqn"} is @qcode{"on"}, @code{fsolve} will attempt to solve ## complex equations in complex variables, assuming that the equations possess
--- a/scripts/optimization/fzero.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/optimization/fzero.m Sun Mar 27 15:50:01 2016 -0700 @@ -76,10 +76,12 @@ ## Number of function evaluations. ## ## @item bracketx -## A two-element vector with the final bracketing of the zero along the x-axis. +## A two-element vector with the final bracketing of the zero along the +## x-axis. ## ## @item brackety -## A two-element vector with the final bracketing of the zero along the y-axis. +## A two-element vector with the final bracketing of the zero along the +## y-axis. ## @end itemize ## @seealso{optimset, fsolve} ## @end deftypefn
--- a/scripts/pkg/pkg.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/pkg/pkg.m Sun Mar 27 15:50:01 2016 -0700 @@ -168,7 +168,8 @@ ## ## @item describe ## Show a short description of the named installed packages, with the option -## @qcode{"-verbose"} also list functions provided by the package. For example, +## @qcode{"-verbose"} also list functions provided by the package. For +## example, ## ## @example ## pkg describe -verbose all @@ -270,8 +271,8 @@ ## @item rebuild ## Rebuild the package database from the installed directories. This can ## be used in cases where the package database has been corrupted. -## It can also take the @option{-auto} and @option{-noauto} options to allow the -## autoloading state of a package to be changed. For example, +## It can also take the @option{-auto} and @option{-noauto} options to allow +## the autoloading state of a package to be changed. For example, ## ## @example ## pkg rebuild -noauto image
--- a/scripts/pkg/private/build.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/pkg/private/build.m Sun Mar 27 15:50:01 2016 -0700 @@ -25,7 +25,9 @@ ## ## @enumerate ## @item untar the tarball in @var{builddir}; +## ## @item build anything necessary (configure and make); +## ## @item repackage specifying the build arch in the tarball filename. ## @end enumerate ##
--- a/scripts/plot/appearance/specular.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/appearance/specular.m Sun Mar 27 15:50:01 2016 -0700 @@ -28,8 +28,8 @@ ## given as 2-element vectors [azimuth, elevation] in degrees or as 3-element ## vectors [x, y, z]. ## -## An optional sixth argument specifies the specular exponent (spread) @var{se}. -## If not given, @var{se} defaults to 10. +## An optional sixth argument specifies the specular exponent (spread) +## @var{se}. If not given, @var{se} defaults to 10. ## @seealso{diffuse, surfl} ## @end deftypefn
--- a/scripts/plot/appearance/view.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/appearance/view.m Sun Mar 27 15:50:01 2016 -0700 @@ -39,7 +39,8 @@ ## If the first argument @var{hax} is an axes handle, then operate on ## this axis rather than the current axes returned by @code{gca}. ## -## If no inputs are given, return the current @var{azimuth} and @var{elevation}. +## If no inputs are given, return the current @var{azimuth} and +## @var{elevation}. ## @end deftypefn ## Author: jwe
--- a/scripts/plot/draw/bar.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/bar.m Sun Mar 27 15:50:01 2016 -0700 @@ -40,7 +40,8 @@ ## ## @table @asis ## @item @qcode{"grouped"} (default) -## Side-by-side bars with a gap between bars and centered over the X-coordinate. +## Side-by-side bars with a gap between bars and centered over the +## X-coordinate. ## ## @item @qcode{"stacked"} ## Bars are stacked so that each X value has a single bar composed of
--- a/scripts/plot/draw/barh.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/barh.m Sun Mar 27 15:50:01 2016 -0700 @@ -40,7 +40,8 @@ ## ## @table @asis ## @item @qcode{"grouped"} (default) -## Side-by-side bars with a gap between bars and centered over the Y-coordinate. +## Side-by-side bars with a gap between bars and centered over the +## Y-coordinate. ## ## @item @qcode{"stacked"} ## Bars are stacked so that each Y value has a single bar composed of
--- a/scripts/plot/draw/contour3.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/contour3.m Sun Mar 27 15:50:01 2016 -0700 @@ -42,7 +42,8 @@ ## If the first argument @var{hax} is an axes handle, then plot into this axis, ## rather than the current axes returned by @code{gca}. ## -## The optional output @var{c} are the contour levels in @code{contourc} format. +## The optional output @var{c} are the contour levels in @code{contourc} +## format. ## ## The optional return value @var{h} is a graphics handle to the hggroup ## comprising the contour lines.
--- a/scripts/plot/draw/isosurface.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/isosurface.m Sun Mar 27 15:50:01 2016 -0700 @@ -42,8 +42,8 @@ ## ## The string input argument @qcode{"noshare"} is only for compatibility and ## has no effect. If given the string input argument -## @qcode{"verbose"} then print messages to the command line interface about the -## current progress. +## @qcode{"verbose"} then print messages to the command line interface about +## the current progress. ## ## If called with the input argument @var{col} which is a ## three-dimensional array of the same size than @var{val} then take
--- a/scripts/plot/draw/line.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/line.m Sun Mar 27 15:50:01 2016 -0700 @@ -34,8 +34,8 @@ ## If the first argument @var{hax} is an axes handle, then plot into this axis, ## rather than the current axes returned by @code{gca}. ## -## The optional return value @var{h} is a graphics handle (or vector of handles) -## to the line objects created. +## The optional return value @var{h} is a graphics handle (or vector of +## handles) to the line objects created. ## ## @seealso{image, patch, rectangle, surface, text} ## @end deftypefn
--- a/scripts/plot/draw/pie.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/pie.m Sun Mar 27 15:50:01 2016 -0700 @@ -42,9 +42,9 @@ ## and text objects generating the plot. ## ## Note: If @code{sum (@var{x}) @leq{} 1} then the elements of @var{x} are -## interpreted as percentages directly and are not normalized by @code{sum (x)}. -## Furthermore, if the sum is less than 1 then there will be a missing slice -## in the pie plot to represent the missing, unspecified percentage. +## interpreted as percentages directly and are not normalized by @code{sum +## (x)}. Furthermore, if the sum is less than 1 then there will be a missing +## slice in the pie plot to represent the missing, unspecified percentage. ## ## @seealso{pie3, bar, hist, rose} ## @end deftypefn
--- a/scripts/plot/draw/pie3.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/pie3.m Sun Mar 27 15:50:01 2016 -0700 @@ -43,9 +43,9 @@ ## patch, surface, and text objects generating the plot. ## ## Note: If @code{sum (@var{x}) @leq{} 1} then the elements of @var{x} are -## interpreted as percentages directly and are not normalized by @code{sum (x)}. -## Furthermore, if the sum is less than 1 then there will be a missing slice -## in the pie plot to represent the missing, unspecified percentage. +## interpreted as percentages directly and are not normalized by @code{sum +## (x)}. Furthermore, if the sum is less than 1 then there will be a missing +## slice in the pie plot to represent the missing, unspecified percentage. ## ## @seealso{pie, bar, hist, rose} ## @end deftypefn
--- a/scripts/plot/draw/quiver3.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/quiver3.m Sun Mar 27 15:50:01 2016 -0700 @@ -42,8 +42,8 @@ ## The style to use for the plot can be defined with a line style @var{style} ## of the same format as the @code{plot} command. ## If a marker is specified then markers at the grid points of the vectors are -## drawn rather than arrows. If the argument @qcode{"filled"} is given then the -## markers are filled. +## drawn rather than arrows. If the argument @qcode{"filled"} is given then +## the markers are filled. ## ## If the first argument @var{hax} is an axes handle, then plot into this axis, ## rather than the current axes returned by @code{gca}.
--- a/scripts/plot/draw/scatter.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/scatter.m Sun Mar 27 15:50:01 2016 -0700 @@ -38,8 +38,8 @@ ## The color of the markers is determined by @var{c}, which can be a string ## defining a fixed color; a 3-element vector giving the red, green, and blue ## components of the color; a vector of the same length as @var{x} that gives -## a scaled index into the current colormap; or an @nospell{Nx3} matrix defining -## the RGB color of each marker individually. +## a scaled index into the current colormap; or an @nospell{Nx3} matrix +## defining the RGB color of each marker individually. ## ## The marker to use can be changed with the @var{style} argument, that is a ## string defining a marker in the same manner as the @code{plot} command.
--- a/scripts/plot/draw/scatter3.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/scatter3.m Sun Mar 27 15:50:01 2016 -0700 @@ -38,8 +38,8 @@ ## The color of the markers is determined by @var{c}, which can be a string ## defining a fixed color; a 3-element vector giving the red, green, and blue ## components of the color; a vector of the same length as @var{x} that gives -## a scaled index into the current colormap; or an @nospell{Nx3} matrix defining -## the RGB color of each marker individually. +## a scaled index into the current colormap; or an @nospell{Nx3} matrix +## defining the RGB color of each marker individually. ## ## The marker to use can be changed with the @var{style} argument, that is a ## string defining a marker in the same manner as the @code{plot} command.
--- a/scripts/plot/draw/stem3.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/stem3.m Sun Mar 27 15:50:01 2016 -0700 @@ -27,7 +27,8 @@ ## ## Stems are drawn from the height @var{z} to the location in the x-y plane ## determined by @var{x} and @var{y}. The default color is @qcode{"b"} (blue), -## the default line style is @qcode{"-"}, and the default marker is @qcode{"o"}. +## the default line style is @qcode{"-"}, and the default marker is +## @qcode{"o"}. ## ## The line style can be altered by the @code{linespec} argument in the same ## manner as the @code{plot} command. If the @qcode{"filled"} argument is
--- a/scripts/plot/draw/stemleaf.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/stemleaf.m Sun Mar 27 15:50:01 2016 -0700 @@ -71,7 +71,8 @@ ## @code{@var{xs} = sort (@var{x})} before calling @code{stemleaf (@var{xs})}. ## ## The stem and leaf plot and associated displays are described in: -## Ch. 3, @cite{Exploratory Data Analysis} by J. W. Tukey, Addison-Wesley, 1977. +## Chapter 3, @cite{Exploratory Data Analysis} by J. W. Tukey, Addison-Wesley, +## 1977. ## @seealso{hist, printd} ## @end deftypefn
--- a/scripts/plot/draw/surfl.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/surfl.m Sun Mar 27 15:50:01 2016 -0700 @@ -41,9 +41,9 @@ ## @strong{Warning:} The alternative mode @qcode{"light"} mode which creates a ## light object to illuminate the surface is not implemented (yet). ## -## The light source location can be specified using @var{lsrc}. It can be given -## as a 2-element vector [azimuth, elevation] in degrees, or as a 3-element -## vector [lx, ly, lz]. The default value is rotated 45 degrees +## The light source location can be specified using @var{lsrc}. It can be +## given as a 2-element vector [azimuth, elevation] in degrees, or as a +## 3-element vector [lx, ly, lz]. The default value is rotated 45 degrees ## counterclockwise to the current view. ## ## The material properties of the surface can specified using a 4-element
--- a/scripts/plot/draw/tetramesh.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/draw/tetramesh.m Sun Mar 27 15:50:01 2016 -0700 @@ -21,7 +21,8 @@ ## @deftypefnx {} {} tetramesh (@var{T}, @var{X}, @var{C}) ## @deftypefnx {} {} tetramesh (@dots{}, @var{property}, @var{val}, @dots{}) ## @deftypefnx {} {@var{h} =} tetramesh (@dots{}) -## Display the tetrahedrons defined in the m-by-4 matrix @var{T} as 3-D patches. +## Display the tetrahedrons defined in the m-by-4 matrix @var{T} as 3-D +## patches. ## ## @var{T} is typically the output of a Delaunay triangulation of a 3-D set ## of points. Every row of @var{T} contains four indices into the n-by-3
--- a/scripts/plot/util/isfigure.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/plot/util/isfigure.m Sun Mar 27 15:50:01 2016 -0700 @@ -21,7 +21,8 @@ ## Return true if @var{h} is a figure graphics handle and false otherwise. ## ## If @var{h} is a matrix then return a logical array which is true where the -## elements of @var{h} are figure graphics handles and false where they are not. +## elements of @var{h} are figure graphics handles and false where they are +## not. ## @seealso{isaxes, ishandle} ## @end deftypefn
--- a/scripts/polynomial/mkpp.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/polynomial/mkpp.m Sun Mar 27 15:50:01 2016 -0700 @@ -33,12 +33,12 @@ ## coefficients for the polynomial over the @var{i}-th interval, ordered from ## highest (@var{m}) to lowest (@var{0}). ## -## @var{coefs} may also be a multi-dimensional array, specifying a vector-valued -## or array-valued polynomial. In that case the polynomial order is defined -## by the length of the last dimension of @var{coefs}. The size of first -## dimension(s) are given by the scalar or vector @var{d}. If @var{d} is not -## given it is set to @code{1}. In any case @var{coefs} is reshaped to a 2-D -## matrix of size @code{[@var{ni}*prod(@var{d} @var{m})] } +## @var{coefs} may also be a multi-dimensional array, specifying a +## vector-valued or array-valued polynomial. In that case the polynomial +## order is defined by the length of the last dimension of @var{coefs}. The +## size of first dimension(s) are given by the scalar or vector @var{d}. If +## @var{d} is not given it is set to @code{1}. In any case @var{coefs} is +## reshaped to a 2-D matrix of size @code{[@var{ni}*prod(@var{d} @var{m})]}. ## ## @seealso{unmkpp, ppval, spline, pchip, ppder, ppint, ppjumps} ## @end deftypefn
--- a/scripts/polynomial/pchip.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/polynomial/pchip.m Sun Mar 27 15:50:01 2016 -0700 @@ -51,7 +51,8 @@ ## @code{@var{s1} * @var{s2} * @dots{} * @var{sk}} ## @end ifnottex ## and each row of this matrix is then treated separately. Note that this is -## exactly opposite to @code{interp1} but is done for @sc{matlab} compatibility. +## exactly opposite to @code{interp1} but is done for @sc{matlab} +## compatibility. ## ## @seealso{spline, ppval, mkpp, unmkpp} ## @end deftypefn
--- a/scripts/polynomial/residue.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/polynomial/residue.m Sun Mar 27 15:50:01 2016 -0700 @@ -87,8 +87,8 @@ ## polynomial specified by @var{r}, @var{p} and @var{k}, and the pole ## multiplicity @var{e}. ## -## If the multiplicity, @var{e}, is not explicitly specified the multiplicity is -## determined by the function @code{mpoles}. +## If the multiplicity, @var{e}, is not explicitly specified the +## multiplicity is determined by the function @code{mpoles}. ## ## For example: ##
--- a/scripts/polynomial/splinefit.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/polynomial/splinefit.m Sun Mar 27 15:50:01 2016 -0700 @@ -31,9 +31,9 @@ ## @var{x} is a vector, and @var{y} is a vector or N-D array. If @var{y} is an ## N-D array, then @var{x}(j) is matched to @var{y}(:,@dots{},:,j). ## -## @var{p} is a positive integer defining the number of intervals along @var{x}, -## and @var{p}+1 is the number of breaks. The number of points in each interval -## differ by no more than 1. +## @var{p} is a positive integer defining the number of intervals along +## @var{x}, and @var{p}+1 is the number of breaks. The number of points in +## each interval differ by no more than 1. ## ## The optional property @var{periodic} is a logical value which specifies ## whether a periodic boundary condition is applied to the spline. The
--- a/scripts/prefs/rmpref.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/prefs/rmpref.m Sun Mar 27 15:50:01 2016 -0700 @@ -20,7 +20,8 @@ ## @deftypefn {} {} rmpref ("@var{group}", "@var{pref}") ## @deftypefnx {} {} rmpref ("@var{group}", @{"@var{pref1}", "@var{pref2}", @dots{}@}) ## @deftypefnx {} {} rmpref ("@var{group}") -## Remove the named preference @var{pref} from the preference group @var{group}. +## Remove the named preference @var{pref} from the preference group +## @var{group}. ## ## The named preference group must be a string. ##
--- a/scripts/set/unique.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/set/unique.m Sun Mar 27 15:50:01 2016 -0700 @@ -26,7 +26,8 @@ ## Return the unique elements of @var{x} sorted in ascending order. ## ## If the input @var{x} is a column vector then return a column vector; -## Otherwise, return a row vector. @var{x} may also be a cell array of strings. +## Otherwise, return a row vector. @var{x} may also be a cell array of +## strings. ## ## If the optional argument @qcode{"rows"} is given then return the unique ## rows of @var{x} sorted in ascending order. The input must be a 2-D matrix @@ -35,10 +36,11 @@ ## If requested, return index vectors @var{i} and @var{j} such that ## @code{@var{y} = @var{x}(@var{i})} and @code{@var{x} = @var{y}(@var{j})}. ## -## Additionally, if @var{i} is a requested output then one of @qcode{"first"} or -## @qcode{"last"} may be given as an input. If @qcode{"last"} is specified, -## return the highest possible indices in @var{i}, otherwise, if @qcode{"first"} -## is specified, return the lowest. The default is @qcode{"last"}. +## Additionally, if @var{i} is a requested output then one of +## @qcode{"first"} or @qcode{"last"} may be given as an input. If +## @qcode{"last"} is specified, return the highest possible indices in +## @var{i}, otherwise, if @qcode{"first"} is specified, return the lowest. +## The default is @qcode{"last"}. ## @seealso{union, intersect, setdiff, setxor, ismember} ## @end deftypefn
--- a/scripts/sparse/eigs.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/sparse/eigs.m Sun Mar 27 15:50:01 2016 -0700 @@ -107,7 +107,8 @@ ## @table @code ## @item issym ## If @var{af} is given, then flags whether the function @var{af} defines a -## symmetric problem. It is ignored if @var{A} is given. The default is false. +## symmetric problem. It is ignored if @var{A} is given. The default is +## false. ## ## @item isreal ## If @var{af} is given, then flags whether the function @var{af} defines a @@ -173,13 +174,13 @@ ## @end table ## ## The return arguments of @code{eigs} depend on the number of return arguments -## requested. With a single return argument, a vector @var{d} of length @var{k} -## is returned containing the @var{k} eigenvalues that have been found. With -## two return arguments, @var{V} is a @var{n}-by-@var{k} matrix whose columns -## are the @var{k} eigenvectors corresponding to the returned eigenvalues. The -## eigenvalues themselves are returned in @var{d} in the form of a -## @var{n}-by-@var{k} matrix, where the elements on the diagonal are the -## eigenvalues. +## requested. With a single return argument, a vector @var{d} of length +## @var{k} is returned containing the @var{k} eigenvalues that have been +## found. With two return arguments, @var{V} is a @var{n}-by-@var{k} matrix +## whose columns are the @var{k} eigenvectors corresponding to the returned +## eigenvalues. The eigenvalues themselves are returned in @var{d} in the +## form of a @var{n}-by-@var{k} matrix, where the elements on the diagonal +## are the eigenvalues. ## ## Given a third return argument @var{flag}, @code{eigs} returns the status ## of the convergence. If @var{flag} is 0 then all eigenvalues have converged.
--- a/scripts/sparse/ilu.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/sparse/ilu.m Sun Mar 27 15:50:01 2016 -0700 @@ -154,7 +154,8 @@ ## @end example ## ## This example uses ILU as preconditioner for a random FEM-Matrix, which has a -## large condition number. Without @var{L} and @var{U} BICG would not converge. +## large condition number. Without @var{L} and @var{U} BICG would not +## converge. ## ## @seealso{lu, ichol, bicg, gmres} ## @end deftypefn
--- a/scripts/specfun/factor.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/specfun/factor.m Sun Mar 27 15:50:01 2016 -0700 @@ -26,7 +26,8 @@ ## return 1. ## ## With two output arguments, return the unique prime factors @var{pf} and -## their multiplicities. That is, @code{prod (@var{pf} .^ @var{n}) == @var{q}}. +## their multiplicities. That is, +## @code{prod (@var{pf} .^ @var{n}) == @var{q}}. ## ## Implementation Note: The input @var{q} must be less than ## @code{flintmax} (9.0072e+15) in order to factor correctly.
--- a/scripts/specfun/factorial.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/specfun/factorial.m Sun Mar 27 15:50:01 2016 -0700 @@ -18,7 +18,8 @@ ## -*- texinfo -*- ## @deftypefn {} {} factorial (@var{n}) -## Return the factorial of @var{n} where @var{n} is a real non-negative integer. +## Return the factorial of @var{n} where @var{n} is a real non-negative +## integer. ## ## If @var{n} is a scalar, this is equivalent to @code{prod (1:@var{n})}. For ## vector or matrix arguments, return the factorial of each element in the
--- a/scripts/special-matrix/gallery.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/special-matrix/gallery.m Sun Mar 27 15:50:01 2016 -0700 @@ -154,8 +154,8 @@ ## If @var{imin} is given then the integers are in the range ## [@var{imin}, @var{imax}]. ## -## The second input is a matrix of dimensions describing the size of the output. -## The dimensions can also be input as comma-separated arguments. +## The second input is a matrix of dimensions describing the size of the +## output. The dimensions can also be input as comma-separated arguments. ## ## The input @var{j} is an integer index in the range [0, 2^32-1]. The values ## of the output matrix are always exactly the same (reproducibility) for a
--- a/scripts/special-matrix/hankel.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/special-matrix/hankel.m Sun Mar 27 15:50:01 2016 -0700 @@ -24,7 +24,8 @@ ## ## If the last element of @var{c} is not the same as the first element of ## @var{r}, the last element of @var{c} is used. If the second argument is -## omitted, it is assumed to be a vector of zeros with the same size as @var{c}. +## omitted, it is assumed to be a vector of zeros with the same size as +## @var{c}. ## ## A Hankel matrix formed from an m-vector @var{c}, and an n-vector @var{r}, ## has the elements
--- a/scripts/statistics/base/histc.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/statistics/base/histc.m Sun Mar 27 15:50:01 2016 -0700 @@ -24,10 +24,10 @@ ## Compute histogram counts. ## ## When @var{x} is a vector, the function counts the number of elements of -## @var{x} that fall in the histogram bins defined by @var{edges}. This must be -## a vector of monotonically increasing values that define the edges of the -## histogram bins. @code{@var{n}(k)} contains the number of elements in -## @var{x} for which @code{@var{edges}(k) <= @var{x} < @var{edges}(k+1)}. +## @var{x} that fall in the histogram bins defined by @var{edges}. This +## must be a vector of monotonically increasing values that define the edges +## of the histogram bins. @code{@var{n}(k)} contains the number of elements +## in @var{x} for which @code{@var{edges}(k) <= @var{x} < @var{edges}(k+1)}. ## The final element of @var{n} contains the number of elements of @var{x} ## exactly equal to the last element of @var{edges}. ## @@ -36,9 +36,9 @@ ## first non-singleton dimension. ## ## When a second output argument is requested an index matrix is also returned. -## The @var{idx} matrix has the same size as @var{x}. Each element of @var{idx} -## contains the index of the histogram bin in which the corresponding element -## of @var{x} was counted. +## The @var{idx} matrix has the same size as @var{x}. Each element of +## @var{idx} contains the index of the histogram bin in which the +## corresponding element of @var{x} was counted. ## @seealso{hist} ## @end deftypefn
--- a/scripts/statistics/base/ols.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/statistics/base/ols.m Sun Mar 27 15:50:01 2016 -0700 @@ -41,7 +41,8 @@ ## @math{t} by @math{p} matrix. ## @end ifnottex ## -## Each row of @var{y} and @var{x} is an observation and each column a variable. +## Each row of @var{y} and @var{x} is an observation and each column a +## variable. ## ## The return values @var{beta}, @var{sigma}, and @var{r} are defined as ## follows.
--- a/scripts/statistics/distributions/finv.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/statistics/distributions/finv.m Sun Mar 27 15:50:01 2016 -0700 @@ -20,7 +20,8 @@ ## -*- texinfo -*- ## @deftypefn {} {} finv (@var{x}, @var{m}, @var{n}) ## For each element of @var{x}, compute the quantile (the inverse of the CDF) -## at @var{x} of the F distribution with @var{m} and @var{n} degrees of freedom. +## at @var{x} of the F distribution with @var{m} and @var{n} degrees of +## freedom. ## @end deftypefn ## Author: KH <Kurt.Hornik@wu-wien.ac.at>
--- a/scripts/statistics/distributions/fpdf.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/statistics/distributions/fpdf.m Sun Mar 27 15:50:01 2016 -0700 @@ -20,7 +20,8 @@ ## -*- texinfo -*- ## @deftypefn {} {} fpdf (@var{x}, @var{m}, @var{n}) ## For each element of @var{x}, compute the probability density function (PDF) -## at @var{x} of the F distribution with @var{m} and @var{n} degrees of freedom. +## at @var{x} of the F distribution with @var{m} and @var{n} degrees of +## freedom. ## @end deftypefn ## Author: KH <Kurt.Hornik@wu-wien.ac.at>
--- a/scripts/statistics/tests/kruskal_wallis_test.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/statistics/tests/kruskal_wallis_test.m Sun Mar 27 15:50:01 2016 -0700 @@ -37,7 +37,8 @@ ## total number of values in the input data. For more info on this ## adjustment see @nospell{William H. Kruskal and W. Allen Wallis}, ## @cite{Use of Ranks in One-Criterion Variance Analysis}, -## Journal of the American Statistical Association, Vol. 47, No. 260 (Dec 1952). +## Journal of the American Statistical Association, Vol. 47, No. 260 (Dec +## 1952). ## ## The p-value (1 minus the CDF of this distribution at @var{k}) is returned ## in @var{pval}.
--- a/scripts/time/weekday.m Sun Mar 27 15:15:24 2016 -0700 +++ b/scripts/time/weekday.m Sun Mar 27 15:50:01 2016 -0700 @@ -19,7 +19,8 @@ ## -*- texinfo -*- ## @deftypefn {} {[@var{n}, @var{s}] =} weekday (@var{d}) ## @deftypefnx {} {[@var{n}, @var{s}] =} weekday (@var{d}, @var{format}) -## Return the day of the week as a number in @var{n} and as a string in @var{s}. +## Return the day of the week as a number in @var{n} and as a string in +## @var{s}. ## ## The days of the week are numbered 1--7 with the first day being Sunday. ##