--- a/scripts/audio/lin2mu.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/audio/lin2mu.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## If @var{n} is not specified it defaults to 0, 8 or 16 depending on 
 ## the range values in @var{x}.
 ## @end deftypefn
+##
 ## @seealso{mu2lin, loadaudio, saveaudio, playaudio, setaudio, and record}
 
 ## Author: Andreas Weingessel <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/audio/loadaudio.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/audio/loadaudio.m	Tue Oct 19 23:10:55 2004 +0000
@@ -30,6 +30,7 @@
 ## The argument @var{bps} can be either 8 (default) or 16, and specifies
 ## the number of bits per sample used in the audio file.
 ## @end deftypefn
+##
 ## @seealso{lin2mu, mu2lin, saveaudio, playaudio, setaudio, and record}
 
 ## Author: AW <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/audio/mu2lin.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/audio/mu2lin.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## or floating point values in the range -1<=y<=1 if @var{n} is 0.  If
 ## @var{n} is not specified it defaults to 8.
 ## @end deftypefn
+##
 ## @seealso{lin2mu, loadaudio, saveaudio, playaudio, setaudio, and record}
 
 ## Author:  Andreas Weingessel <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/audio/playaudio.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/audio/playaudio.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## Plays the audio file @file{@var{name}.@var{ext}} or the audio data
 ## stored in the vector @var{x}.
 ## @end deftypefn
+##
 ## @seealso{lin2mu, mu2lin, loadaudio, saveaudio, setaudio, and record}
 
 ## Author: AW <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/audio/record.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/audio/record.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## 8kHz.  The program waits until the user types @key{RET} and then
 ## immediately starts to record.
 ## @end deftypefn
+##
 ## @seealso{lin2mu, mu2lin, loadaudio, saveaudio, playaudio, and setaudio}
 
 ## Author: AW <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/audio/saveaudio.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/audio/saveaudio.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## in the audio file (see @code{loadaudio});  defaults are @file{lin} and
 ## 8, respectively.
 ## @end deftypefn
+##
 ## @seealso{lin2mu, mu2lin, loadaudio, playaudio, setaudio, and record}
 
 ## Author: AW <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/control/base/DEMOcontrol.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/DEMOcontrol.m	Tue Oct 19 23:10:55 2004 +0000
@@ -38,6 +38,7 @@
 ## Command examples are interactively run for users to observe the use
 ## of @acronym{OCST} functions.
 ## @end deftypefn
+##
 ## @seealso{Demo Programs: bddemo.m, frdemo.m, analdemo.m,
 ## moddmeo.m, rldemo.m}
 

--- a/scripts/control/base/__stepimp__.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/__stepimp__.m	Tue Oct 19 23:10:55 2004 +0000
@@ -28,6 +28,7 @@
 ## Used internally in @command{impulse}, @command{step}. Use @command{step}
 ## or @command{impulse} instead.
 ## @end deftypefn
+##
 ## @seealso{step, impulse}
 
 ## Author: Kai P. Mueller <mueller@ifr.ing.tu-bs.de>

--- a/scripts/control/base/are.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/are.m	Tue Oct 19 23:10:55 2004 +0000
@@ -61,6 +61,7 @@
 ## matrix.
 ##
 ## @end deftypefn
+##
 ## @seealso{balance and dare}
 
 ## Author: A. S. Hodel <a.s.hodel@eng.auburn.edu>

--- a/scripts/control/base/controldemo.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/controldemo.m	Tue Oct 19 23:10:55 2004 +0000
@@ -20,6 +20,7 @@
 ## @deftypefn {Function File} {} controldemo ()
 ## Control Systems Toolbox demo.
 ## @end deftypefn
+##
 ## @seealso{Demo programs: bddemo, frdemo, analdemo, moddmeo, rldemo}
 
 ## Author: David Clem

--- a/scripts/control/base/damp.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/damp.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## If @var{p} is a matrix and @var{tsam} is specified, eigenvalues
 ## of @var{p} are assumed to be in @var{z}-domain.
 ## @end deftypefn
+##
 ## @seealso{eig}
 
 ## Author: Kai P. Mueller <mueller@ifr.ing.tu-bs.de>

--- a/scripts/control/base/dare.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/dare.m	Tue Oct 19 23:10:55 2004 +0000
@@ -71,6 +71,7 @@
 ##  Systems, Vol 5, no 2 (1992), pp 165--194.
 ##
 ## @end deftypefn
+##
 ## @seealso{balance and are}
 
 ## Author: A. S. Hodel <a.s.hodel@eng.auburn.edu>

--- a/scripts/control/base/impulse.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/impulse.m	Tue Oct 19 23:10:55 2004 +0000
@@ -46,6 +46,7 @@
 ## Times of the impulse response.
 ## @end table
 ## @end deftypefn
+##
 ## @seealso{step, __stepimp__}
 
 ## Author: Kai P. Mueller <mueller@ifr.ing.tu-bs.de>

--- a/scripts/control/base/lqg.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/lqg.m	Tue Oct 19 23:10:55 2004 +0000
@@ -61,6 +61,7 @@
 ## Controller poles.
 ## @end table
 ## @end deftypefn
+##
 ## @seealso{h2syn, lqe, and lqr}
 
 ## Author: A. S. Hodel <a.s.hodel@eng.auburn.edu>

--- a/scripts/control/base/step.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/base/step.m	Tue Oct 19 23:10:55 2004 +0000
@@ -48,6 +48,7 @@
 ##
 ## When invoked with the output parameter @var{y} the plot is not displayed.
 ## @end deftypefn
+##
 ## @seealso{impulse and __stepimp__}
 
 ## Author: Kai P. Mueller <mueller@ifr.ing.tu-bs.de>

--- a/scripts/control/system/abcddim.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/abcddim.m	Tue Oct 19 23:10:55 2004 +0000
@@ -59,6 +59,7 @@
 ## Note: n = 0 (pure gain block) is returned without warning.
 ##
 ## @end deftypefn
+##
 ## @seealso{is_abcd}
 
 ## Author: A. S. Hodel <a.s.hodel@eng.auburn.edu>

--- a/scripts/control/system/is_abcd.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/is_abcd.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ##  appropriate diagnostic message printed to the screen.  The matrices
 ##  @var{b}, @var{c}, or @var{d} may be omitted.
 ## @end deftypefn
+##
 ## @seealso{abcddim}
 
 ## Author: Kai P. Mueller <mueller@ifr.ing.tu-bs.de>

--- a/scripts/control/system/is_controllable.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/is_controllable.m	Tue Oct 19 23:10:55 2004 +0000
@@ -53,6 +53,7 @@
 ## has a single input; otherwise a block Arnoldi iteration is performed
 ## with @code{krylovb}.
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, ismatrix, isscalar, isvector
 ## is_observable, is_stabilizable, is_detectable, krylov, and krylovb}
 

--- a/scripts/control/system/is_detectable.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/is_detectable.m	Tue Oct 19 23:10:55 2004 +0000
@@ -30,6 +30,7 @@
 ##
 ##
 ## @end deftypefn
+##
 ## @seealso{is_stabilizable, size, rows, columns, length, ismatrix,
 ## isscalar, and isvector}
 

--- a/scripts/control/system/is_observable.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/is_observable.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## See @command{is_controllable} for detailed description of arguments
 ## and default values.
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, ismatrix, isscalar, and isvector}
 
 ## Author: A. S. Hodel <a.s.hodel@eng.auburn.edu>

--- a/scripts/control/system/is_stabilizable.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/is_stabilizable.m	Tue Oct 19 23:10:55 2004 +0000
@@ -35,6 +35,7 @@
 ## @end ifinfo
 ## assume that discrete-time matrices (a,b) are supplied.
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, ismatrix, isscalar, isvector
 ## is_observable, is_stabilizable, is_detectable}
 

--- a/scripts/control/system/is_stable.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/is_stable.m	Tue Oct 19 23:10:55 2004 +0000
@@ -37,6 +37,7 @@
 ## @end table
 ## @end table
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, ismatrix, isscalar, isvector
 ## is_observable, is_stabilizable, is_detectable, krylov, and krylovb}
 

--- a/scripts/control/system/jet707.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/jet707.m	Tue Oct 19 23:10:55 2004 +0000
@@ -35,6 +35,7 @@
 ##
 ## @strong{Reference}: R. Brockhaus: @cite{Flugregelung} (Flight Control), Springer, 1994.
 ## @end deftypefn
+##
 ## @seealso{ord2}
 
 ## Author: Kai P. Mueller <mueller@ifr.ing.tu-bs.de>

--- a/scripts/control/system/sys2fir.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/sys2fir.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## Extract @acronym{FIR} data from system data structure; see @command{fir2sys} for
 ## parameter descriptions.
 ## @end deftypefn
+##
 ## @seealso{fir2sys}
 
 ## Author: A. S. Hodel <a.s.hodel@eng.auburn.edu>

--- a/scripts/control/system/sysdimensions.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/sysdimensions.m	Tue Oct 19 23:10:55 2004 +0000
@@ -63,6 +63,7 @@
 ## @math{yd(ii) = 0} if output @var{ii} is continous
 ## @end table
 ## @end deftypefn
+##
 ## @seealso{sysgetsignals and sysgettsam}
 
 function [n, nz, m, p, yd] = sysdimensions (sys, opt)

--- a/scripts/control/system/sysupdate.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/sysupdate.m	Tue Oct 19 23:10:55 2004 +0000
@@ -48,6 +48,7 @@
 ## Conversion to @command{tf} or @command{zp} exits with an error if the system is
 ## mixed continuous/digital.
 ## @end deftypefn
+##
 ## @seealso{tf, ss, zp, sysout, sys2ss, sys2tf, and sys2zp}
 
 ## Author: John Ingram <ingraje@eng.auburn.edu>

--- a/scripts/control/system/tfout.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/tfout.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## Print formatted transfer function @math{n(s)/d(s)} to the screen.
 ## @var{x} defaults to the string @code{"s"}
 ## @end deftypefn
+##
 ## @seealso{polyval, polyvalm, poly, roots, conv, deconv, residue,
 ## filter, polyderiv, polyinteg, and polyout}
 

--- a/scripts/control/system/ugain.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/ugain.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## Watch out if you are forming sampled systems since @command{ugain}
 ## does not contain a sampling period.
 ## @end deftypefn
+##
 ## @seealso{hinfdemo and jet707}
 
 ## Author: Kai P. Mueller <mueller@ifr.ing.tu-bs.de>

--- a/scripts/control/system/zpout.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/control/system/zpout.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## print formatted zero-pole form to the screen.
 ## @var{x} defaults to the string @code{"s"}
 ## @end deftypefn
+##
 ## @seealso{polyval, polyvalm, poly, roots, conv, deconv, residue,
 ## filter, polyderiv, polyinteg, and polyout}
 

--- a/scripts/elfun/lcm.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/elfun/lcm.m	Tue Oct 19 23:10:55 2004 +0000
@@ -32,9 +32,10 @@
 ## @example
 ## lcm ([a1, ..., ak]).
 ## @end example
+##
+## All elements must be the same size or scalar.
 ## @end deftypefn
 ##
-## All elements must be the same size or scalar.
 ## @seealso{gcd, min, max, ceil, and floor}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/finance/irr.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/finance/irr.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## @code{npv (r, p) = i}.  If the second argument is omitted, a value of
 ## 0 is used.
 ## @end deftypefn
+##
 ## @seealso{npv, pv, and rate}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/finance/nper.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/finance/nper.m	Tue Oct 19 23:10:55 2004 +0000
@@ -32,6 +32,7 @@
 ## Note that the rate @var{r} is specified as a fraction (i.e., 0.05,
 ## not 5 percent).
 ## @end deftypefn
+##
 ## @seealso{pv, pmt, rate, and npv}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/finance/npv.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/finance/npv.m	Tue Oct 19 23:10:55 2004 +0000
@@ -31,6 +31,7 @@
 ## Note that the rate @var{r} is specified as a fraction (i.e., 0.05,
 ## not 5 percent).
 ## @end deftypefn
+##
 ## @seealso{irr and pv}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/finance/pmt.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/finance/pmt.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## payments are made at the end (@var{"e"}, default) or at the beginning
 ## (@var{"b"}) of each period.
 ## @end deftypefn
+##
 ## @seealso{pv, nper, and rate}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/finance/pv.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/finance/pv.m	Tue Oct 19 23:10:55 2004 +0000
@@ -32,6 +32,7 @@
 ## Note that the rate @var{r} is specified as a fraction (i.e., 0.05,
 ## not 5 percent).
 ## @end deftypefn
+##
 ## @seealso{pmt, nper, rate, and npv}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/finance/rate.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/finance/rate.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## whether payments are made at the end (@code{"e"}, default) or at the
 ## beginning (@code{"b"}) of each period.
 ## @end deftypefn
+##
 ## @seealso{pv, pmt, nper, and npv}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/general/bitcmp.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/bitcmp.m	Tue Oct 19 23:10:55 2004 +0000
@@ -27,9 +27,9 @@
 ## dec2bin(bitcmp(11))
 ## @result{} 11111111111111111111111111110100
 ## @end example
+## @end deftypefn
 ##
 ## @seealso{bitand,bitor,bitxor,bitset,bitget,bitcmp,bitshift,bitmax}
-## @end deftypefn
 
 ## Liberally based of the version by Kai Habel from octave-forge
 

--- a/scripts/general/bitget.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/bitget.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,8 +23,9 @@
 ## bitget (100, 8:-1:1)
 ## @result{} 0  1  1  0  0  1  0  0 
 ## @end example
+## @end deftypefn
+##
 ## @seealso{bitand, bitor, bitxor, bitset, bitcmp, bitshift, bitmax}
-## @end deftypefn
 
 ## Liberally based of the version by Kai Habel from octave-forge
 

--- a/scripts/general/bitset.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/bitset.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,9 +25,9 @@
 ## dec2bin (bitset (10, 1))
 ## @result{} 1011
 ## @end example
+## @end deftypefn
 ##
 ## @seealso{bitand, bitor, bitxor, bitget, bitcmp, bitshift, bitmax}
-## @end deftypefn
 
 ## Liberally based of the version by Kai Habel from octave-forge
 

--- a/scripts/general/cart2pol.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/cart2pol.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## @var{theta} describes the angle relative to the x - axis.
 ## @var{r} is the distance to the z - axis (0, 0, z).
 ## @end deftypefn
+##
 ## @seealso{pol2cart, cart2sph, sph2cart}
 
 ## Author: Kai Habel <kai.habel@gmx.de>

--- a/scripts/general/cart2sph.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/cart2sph.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## @var{phi} is the angle relative to the xy - plane.
 ## @var{r} is the distance to the origin (0, 0, 0).
 ## @end deftypefn
+##
 ## @seealso{pol2cart, cart2pol, sph2cart}
 
 ## Author: Kai Habel <kai.habel@gmx.de>

--- a/scripts/general/circshift.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/circshift.m	Tue Oct 19 23:10:55 2004 +0000
@@ -44,6 +44,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso {permute, ipermute, shiftdim}
 
 function y = circshift (x, n)

--- a/scripts/general/columns.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/columns.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} columns (@var{a})
 ## Return the number of columns of @var{a}.
 ## @end deftypefn
+##
 ## @seealso{size, rows, length, isscalar, isvector, and ismatrix}
 
 ## Author: jwe

--- a/scripts/general/flipdim.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/flipdim.m	Tue Oct 19 23:10:55 2004 +0000
@@ -30,6 +30,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{fliplr, flipud, rot90 and rotdim}
 
 ## Author: David Bateman

--- a/scripts/general/fliplr.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/fliplr.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,11 +29,11 @@
 ##          4  3
 ## @end group
 ## @end example
+##
+## Note that @code{fliplr} only workw with 2-D arrays.  To flip N-d arrays
+## use @code{flipdim} instead.
 ## @end deftypefn
 ##
-## Due to the difficult of define which axis about which to flip the 
-## matrix @code{fliplr} only work with 2-D arrays. To flip N-D arrays
-## use @code{flipdim} instead.
 ## @seealso{flipud, flipdim, rot90 and rotdim}
 
 ## Author: jwe

--- a/scripts/general/flipud.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/flipud.m	Tue Oct 19 23:10:55 2004 +0000
@@ -34,6 +34,7 @@
 ## matrix @code{flipud} only work with 2-d arrays.  To flip N-d arrays
 ## use @code{flipdim} instead.
 ## @end deftypefn
+##
 ## @seealso{fliplr, flipdim, rot90 and rotdim}
 
 ## Author: jwe

--- a/scripts/general/ind2sub.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/ind2sub.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {[@var{s1}, @var{s2}, @dots{}, @var{sN}] =} ind2sub (@var{dims}, @var{ind})
 ## Convert a linear index into subscripts.
 ## @end deftypefn
+##
 ## @seealso{sub2ind}
 
 ## Author: Paul Kienzle <pkienzle@kienzle.powernet.co.uk>

--- a/scripts/general/int2str.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/int2str.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## but are provided for compatibility with @sc{Matlab}.  For better control
 ## over the results, use @code{sprintf} (@pxref{Formatted Output}).
 ## @end deftypefn
+##
 ## @seealso{sprintf and num2str}
 
 ## Author: jwe

--- a/scripts/general/isdefinite.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/isdefinite.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## positive semidefinite.  Otherwise, return -1.  If @var{tol}
 ## is omitted, use a tolerance equal to 100 times the machine precision.  
 ## @end deftypefn
+##
 ## @seealso{issymmetric}
 
 ## Author: Gabriele Pannocchia <g.pannocchia@ing.unipi.it>

--- a/scripts/general/isscalar.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/isscalar.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} isscalar (@var{a})
 ## Return 1 if @var{a} is a scalar.  Otherwise, return 0.
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, isscalar, and ismatrix}
 
 ## Author: jwe

--- a/scripts/general/issquare.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/issquare.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## If @var{x} is a square matrix, then return the dimension of @var{x}.
 ## Otherwise, return 0.
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, ismatrix, isscalar, and isvector}
 
 ## Author: A. S. Hodel <scotte@eng.auburn.edu>

--- a/scripts/general/issymmetric.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/issymmetric.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## then return the dimension of @var{x}.  Otherwise, return 0.  If
 ## @var{tol} is omitted, use a tolerance equal to the machine precision.
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, ismatrix, isscalar,
 ## issquare, and isvector}
 

--- a/scripts/general/isvector.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/isvector.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} isvector (@var{a})
 ## Return 1 if @var{a} is a vector.  Otherwise, return 0.
 ## @end deftypefn
+##
 ## @seealso{size, rows, columns, length, isscalar, and ismatrix}
 
 ## Author: jwe

--- a/scripts/general/logspace.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/logspace.m	Tue Oct 19 23:10:55 2004 +0000
@@ -59,6 +59,7 @@
 ## @end ifinfo
 ## in order to  be compatible with the corresponding @sc{Matlab} function.
 ## @end deftypefn
+##
 ## @seealso{linspace}
 
 ## Author: jwe

--- a/scripts/general/mod.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/mod.m	Tue Oct 19 23:10:55 2004 +0000
@@ -32,6 +32,7 @@
 ## An error message is printed if the dimensions of the arguments do not
 ## agree, or if either of the arguments is complex.
 ## @end deftypefn
+##
 ## @seealso{rem, round}
 
 ## Author: Paul Kienzle <pkienzle@kienzle.powernet.co.uk>

--- a/scripts/general/nextpow2.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/nextpow2.m	Tue Oct 19 23:10:55 2004 +0000
@@ -31,6 +31,7 @@
 ##
 ## If @var{x} is a vector, return @code{nextpow2 (length (@var{x}))}.
 ## @end deftypefn
+##
 ## @seealso{pow2}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/general/num2str.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/num2str.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## but are provided for compatibility with @sc{Matlab}.  For better control
 ## over the results, use @code{sprintf} (@pxref{Formatted Output}).
 ## @end deftypefn
+##
 ## @seealso{sprintf and int2str}
 
 ## Author: jwe

--- a/scripts/general/perror.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/perror.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## useful error messages for those functions that return numeric error
 ## codes.
 ## @end deftypefn
+##
 ## @seealso{strerror}
 
 ## Author: jwe

--- a/scripts/general/pol2cart.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/pol2cart.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## @var{theta} describes the angle relative to the x - axis.
 ## @var{r} is the distance to the z - axis (0, 0, z).
 ## @end deftypefn
+##
 ## @seealso{cart2pol, cart2sph, sph2cart}
 
 ## Author: Kai Habel <kai.habel@gmx.de>

--- a/scripts/general/rem.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/rem.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## An error message is printed if the dimensions of the arguments do not
 ## agree, or if either of the arguments is complex.
 ## @end deftypefn
+##
 ## @seealso{mod, round}
 
 ## Author: jwe

--- a/scripts/general/rot90.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/rot90.m	Tue Oct 19 23:10:55 2004 +0000
@@ -51,6 +51,7 @@
 ## matrix @code{rot90} only work with 2-D arrays.  To rotate N-d arrays
 ## use @code{rotdim} instead.
 ## @end deftypefn
+##
 ## @seealso{rotdim, flipud, fliplr and flipdim}
 
 ## Author: jwe

--- a/scripts/general/rotdim.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/rotdim.m	Tue Oct 19 23:10:55 2004 +0000
@@ -52,6 +52,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{rot90, flipud, fliplr and flipdim}
 
 function y = rotdim (x, k, plane)

--- a/scripts/general/rows.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/rows.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} rows (@var{a})
 ## Return the number of rows of @var{a}.
 ## @end deftypefn
+##
 ## @seealso{size, columns, length, isscalar, isvector, and ismatrix}
 
 ## Author: jwe

--- a/scripts/general/shiftdim.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/shiftdim.m	Tue Oct 19 23:10:55 2004 +0000
@@ -46,6 +46,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso {reshape, permute, ipermute, circshift, squeeze}
 
 function [y, ns]  = shiftdim (x, n)

--- a/scripts/general/sph2cart.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/sph2cart.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## @var{phi} is the angle relative to the xy-plane.
 ## @var{r} is the distance to the origin (0, 0, 0).
 ## @end deftypefn
+##
 ## @seealso{pol2cart, cart2pol, cart2sph}
 
 ## Author: Kai Habel <kai.habel@gmx.de>

--- a/scripts/general/sub2ind.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/sub2ind.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## @deftypefnx {Function File} {@var{ind} =} sub2ind (@var{dims}, @var{s1}, @var{s2}, @dots{}, @var{sN})
 ## Convert subscripts into a linear index.
 ## @end deftypefn
+##
 ## @seealso{ind2sub}
 
 ## Author: Paul Kienzle <pkienzle@kienzle.powernet.co.uk>

--- a/scripts/general/tril.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/general/tril.m	Tue Oct 19 23:10:55 2004 +0000
@@ -60,6 +60,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{triu and diag}
 
 ## Author: jwe

--- a/scripts/image/hsv2rgb.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/hsv2rgb.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} @var{rgb_map} = hsv2rgb (@var{hsv_map})
 ## Transform a colormap from the hsv space to the rgb space. 
 ## @end deftypefn
+##
 ## @seealso{rgb2hsv}
 
 ## Author: Kai Habel <kai.habel@gmx.de>

--- a/scripts/image/image.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/image.m	Tue Oct 19 23:10:55 2004 +0000
@@ -31,6 +31,7 @@
 ## The axis values corresponding to the matrix elements are specified in
 ## @var{x} and @var{y}. At present they are ignored.
 ## @end deftypefn
+##
 ## @seealso{imshow, imagesc, and colormap}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/image/imagesc.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/imagesc.m	Tue Oct 19 23:10:55 2004 +0000
@@ -35,6 +35,7 @@
 ## values for the respective axes, or as values for each row and column
 ## of the matrix @var{A}.  At present they are ignored.
 ## @end deftypefn
+##
 ## @seealso{image and imshow}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/image/ind2gray.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/ind2gray.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## If @var{map} is omitted, the current colormap is used to determine the
 ## intensities.
 ## @end deftypefn
+##
 ## @seealso{gray2ind, rgb2ntsc, image, and colormap}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/image/ind2rgb.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/ind2rgb.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## Convert an indexed image to red, green, and blue color components.
 ## If @var{map} is omitted, the current colormap is used for the conversion.
 ## @end deftypefn
+##
 ## @seealso{rgb2ind, image, imshow, ind2gray, and gray2ind}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/image/loadimage.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/loadimage.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## Load an image file and it's associated color map from the specified
 ## @var{file}.  The image must be stored in Octave's image format.
 ## @end deftypefn
+##
 ## @seealso{saveimage, load, and save}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/image/rgb2hsv.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/rgb2hsv.m	Tue Oct 19 23:10:55 2004 +0000
@@ -28,6 +28,7 @@
 ## Hue describes the dominant wavelegth. 
 ## Saturation is the amount of Hue mixed into the color. 
 ## @end deftypefn
+##
 ## @seealso{hsv2rgb}
 
 ## Author: Kai Habel <kai.habel@gmx.de>

--- a/scripts/image/rgb2ind.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/rgb2ind.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {[@var{x}, @var{map}] =} rgb2ind (@var{r}, @var{g}, @var{b})
 ## Convert and RGB image to an Octave indexed image.
 ## @end deftypefn
+##
 ## @seealso{ind2rgb and rgb2ntsc}
 
 ## Bugs: The color map may have duplicate entries.

--- a/scripts/image/saveimage.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/image/saveimage.m	Tue Oct 19 23:10:55 2004 +0000
@@ -43,6 +43,8 @@
 ## are equal) the gray scale ppm and PostScript image formats are used,
 ## otherwise the full color formats are used.
 ## @end deftypefn
+##
+## @seealso{loadimage, save, load, and colormap}
 
 ## The conversion to PostScript is based on pbmtolps.c, which was
 ## written by
@@ -52,7 +54,6 @@
 ##   University of British Columbia
 ##
 ## and is part of the portable bitmap utilities,
-## @seealso{loadimage, save, load, and colormap}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>
 ## Created: July 1994

--- a/scripts/io/beep.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/io/beep.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} puts (@var{string})
 ## Produce a beep from the speaker (or visual bell).
 ## @end deftypefn
+##
 ## @seealso{puts, fputs, printf and fprintf}
 
 ## Author: jwe

--- a/scripts/linear-algebra/cond.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/linear-algebra/cond.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## defined as @code{norm (a) * norm (inv (a))}, and is computed via a
 ## singular value decomposition.
 ## @end deftypefn
+##
 ## @seealso{norm, svd, and rank}
 
 ## Author: jwe

--- a/scripts/linear-algebra/norm.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/linear-algebra/norm.m	Tue Oct 19 23:10:55 2004 +0000
@@ -53,6 +53,7 @@
 ## p-norm of @var{a}, @code{(sum (abs (@var{a}) .^ @var{p})) ^ (1/@var{p})}.
 ## @end table
 ## @end deftypefn
+##
 ## @seealso{cond and svd}
 
 ## Author: jwe

--- a/scripts/miscellaneous/comma.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/miscellaneous/comma.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,4 +21,5 @@
 ## @deffn {Operator} ,
 ## Array index, function argument, or command separator.
 ## @end deffn
+##
 ## @seealso{semicolon}

--- a/scripts/miscellaneous/dir.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/miscellaneous/dir.m	Tue Oct 19 23:10:55 2004 +0000
@@ -40,6 +40,7 @@
 ## named file.
 ## @var{filename}.
 ## @end deftypefn
+##
 ## @seealso{stat}
 
 ## Author: jwe

--- a/scripts/miscellaneous/etime.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/miscellaneous/etime.m	Tue Oct 19 23:10:55 2004 +0000
@@ -32,6 +32,7 @@
 ## will set the variable @code{elapsed_time} to the number of seconds since
 ## the variable @code{t0} was set.
 ## @end deftypefn
+##
 ## @seealso{tic, toc, clock, and cputime}
 
 ## Author: jwe

--- a/scripts/miscellaneous/menu.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/miscellaneous/menu.m	Tue Oct 19 23:10:55 2004 +0000
@@ -26,6 +26,7 @@
 ## in, but it may be confusing to present more than will fit easily on one
 ## screen.
 ## @end deftypefn
+##
 ## @seealso{disp, printf, and input}
 
 ## Author: jwe

--- a/scripts/miscellaneous/semicolon.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/miscellaneous/semicolon.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,4 +21,5 @@
 ## @deffn {Operator} ;
 ## Array row or command separator.
 ## @end deffn
+##
 ## @seealso{comma}

--- a/scripts/miscellaneous/texas_lotto.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/miscellaneous/texas_lotto.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## Pick 6 unique numbers between 1 and 50 that are guaranteed to win
 ## the Texas Lotto.
 ## @end deftypefn
+##
 ## @seealso{rand}
 
 ## Author: jwe

--- a/scripts/miscellaneous/unix.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/miscellaneous/unix.m	Tue Oct 19 23:10:55 2004 +0000
@@ -26,6 +26,7 @@
 ## @var{text}.  If the optional second argument @code{"-echo"} is given,
 ## then also send the output from the command to the standard output.
 ## @end deftypefn
+##
 ## @seealso{isunix, ispc, system}
 
 ## Author: octave-forge ???

--- a/scripts/plot/__errcomm__.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/__errcomm__.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## semilogyerr, semilogxerr).
 ##
 ## @end deftypefn
+##
 ## @seealso{errorbar, semilogxerr, semilogyerr, loglogerr, __pltopt__}
 
 ## Created: 20.02.2001

--- a/scripts/plot/__errplot__.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/__errplot__.m	Tue Oct 19 23:10:55 2004 +0000
@@ -26,6 +26,7 @@
 ## @end example
 ##
 ## @end deftypefn
+##
 ## @seealso{semilogx, semilogy, loglog, polar, mesh, contour, __pltopt__
 ## bar, stairs, errorbar, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/__pltopt1__.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/__pltopt1__.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} __pltopt1__ (@var{caller}, @var{opt})
 ## Really decode plot option strings.
 ## @end deftypefn
+##
 ## @seealso{__pltopt__}
 
 ## Author: Rick Niles <niles@axp745.gsfc.nasa.gov>

--- a/scripts/plot/__pltopt__.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/__pltopt__.m	Tue Oct 19 23:10:55 2004 +0000
@@ -104,6 +104,7 @@
 ##   6    brown     yellow      dot short dash  "*"         "o"
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{__pltopt1__}
 
 ## Author: jwe

--- a/scripts/plot/bar.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/bar.m	Tue Oct 19 23:10:55 2004 +0000
@@ -42,6 +42,7 @@
 ## @noindent
 ## are equivalent.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, mesh, contour,
 ## stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/contour.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/contour.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## @var{z}.  Someone needs to improve @code{gnuplot}'s contour routines
 ## before this will be very useful.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, mesh, contour,
 ## bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/errorbar.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/errorbar.m	Tue Oct 19 23:10:55 2004 +0000
@@ -103,6 +103,7 @@
 ## from @var{y}-@var{ly} to @var{y}+@var{uy}.
 ##
 ## @end deftypefn
+##
 ## @seealso{semilogx, semilogy, loglog, polar, mesh, contour, __pltopt__,
 ## bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/grid.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/grid.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## The argument may be either @code{"on"} or @code{"off"}.  If it is
 ## omitted, @code{"on"} is assumed.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, mesh, contour,
 ## bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/hist.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/hist.m	Tue Oct 19 23:10:55 2004 +0000
@@ -39,6 +39,7 @@
 ## With two output arguments, produce the values @var{nn} and @var{xx} such
 ## that @code{bar (@var{xx}, @var{nn})} will plot the histogram.
 ## @end deftypefn
+##
 ## @seealso{bar}
 
 ## Author: jwe

--- a/scripts/plot/loglog.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/loglog.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## description of @code{plot} for a description of the arguments that
 ## @code{loglog} will accept.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogy, loglog, polar, mesh, contour, bar, stairs,
 ## gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/loglogerr.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/loglogerr.m	Tue Oct 19 23:10:55 2004 +0000
@@ -34,6 +34,7 @@
 ## additional information.
 ##
 ## @end deftypefn
+##
 ## @seealso{errorbar, semilogxerr, semilogyerr, polar, mesh, contour, 
 ## __pltopt__, bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/mesh.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/mesh.m	Tue Oct 19 23:10:55 2004 +0000
@@ -26,6 +26,7 @@
 ## correspond to different @var{x} values and rows of @var{z} correspond
 ## to different @var{y} values.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, meshgrid, meshdom,
 ## contour, bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/meshgrid.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/meshgrid.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## to the @var{x} and @var{y} coordinates of a mesh.  The rows of @var{xx} are copies of @var{x},
 ## and the columns of @var{yy} are copies of @var{y}.
 ## @end deftypefn
+##
 ## @seealso{sombrero, plot, semilogx, semilogy, loglog, polar, mesh, meshdom, contour,
 ## bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/plot.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/plot.m	Tue Oct 19 23:10:55 2004 +0000
@@ -163,6 +163,7 @@
 ## This will plot the cosine and sine functions and label them accordingly
 ## in the key.
 ## @end deftypefn
+##
 ## @seealso{semilogx, semilogy, loglog, polar, mesh, contour, __pltopt__
 ## bar, stairs, errorbar, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/polar.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/polar.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ##
 ## The optional third argument specifies the line type.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, mesh, contour, bar,
 ## stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/semilogx.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/semilogx.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## the description of @code{plot} for a description of the arguments
 ## that @code{semilogx} will accept.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogy, loglog, polar, mesh, contour, bar, stairs,
 ## gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/semilogxerr.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/semilogxerr.m	Tue Oct 19 23:10:55 2004 +0000
@@ -34,6 +34,7 @@
 ## additional information.
 ##
 ## @end deftypefn
+##
 ## @seealso{errorbar, loglogerr semilogyerr, polar, mesh, contour, __pltopt__, 
 ## bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/semilogy.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/semilogy.m	Tue Oct 19 23:10:55 2004 +0000
@@ -23,6 +23,7 @@
 ## the description of @code{plot} for a description of the arguments
 ## that @code{semilogy} will accept.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, loglog, polar, mesh, contour, bar, stairs,
 ## gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/semilogyerr.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/semilogyerr.m	Tue Oct 19 23:10:55 2004 +0000
@@ -34,6 +34,7 @@
 ## additional information.
 ##
 ## @end deftypefn
+##
 ## @seealso{errorbar, loglogerr semilogxerr, polar, mesh, contour, __pltopt__, 
 ## bar, stairs, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/shg.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/shg.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ## replot without any arguments.
 ##
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, mesh, contour,
 ## bar, stairs, gplot, gsplot, replot, xlabel, and ylabel}
 

--- a/scripts/plot/stairs.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/stairs.m	Tue Oct 19 23:10:55 2004 +0000
@@ -42,6 +42,7 @@
 ## @noindent
 ## are equivalent.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, mesh, contour,
 ## bar, gplot, gsplot, replot, xlabel, ylabel, and title}
 

--- a/scripts/plot/title.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/title.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## Specify a title for a plot.  If you already have a plot displayed, use
 ## the command @code{replot} to redisplay it with the new title.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, mesh, contour,
 ## bar, stairs, gplot, gsplot, replot, xlabel, and ylabel}
 

--- a/scripts/plot/xlabel.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/plot/xlabel.m	Tue Oct 19 23:10:55 2004 +0000
@@ -25,6 +25,7 @@
 ## displayed, use the command @code{replot} to redisplay it with the new
 ## labels.
 ## @end deftypefn
+##
 ## @seealso{plot, semilogx, semilogy, loglog, polar, mesh, contour,
 ## bar, stairs, gplot, gsplot, replot, ylabel, and title}
 

--- a/scripts/polynomial/compan.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/compan.m	Tue Oct 19 23:10:55 2004 +0000
@@ -52,6 +52,7 @@
 ## The eigenvalues of the companion matrix are equal to the roots of the
 ## polynomial.
 ## @end deftypefn
+##
 ## @seealso{poly, roots, residue, conv, deconv, polyval, polyderiv, and
 ## polyinteg}
 

--- a/scripts/polynomial/conv.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/conv.m	Tue Oct 19 23:10:55 2004 +0000
@@ -26,6 +26,7 @@
 ## If @var{a} and @var{b} are polynomial coefficient vectors, @code{conv}
 ## returns the coefficients of the product polynomial.
 ## @end deftypefn
+##
 ## @seealso{deconv, poly, roots, residue, polyval, polyderiv, and polyinteg}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/polynomial/deconv.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/deconv.m	Tue Oct 19 23:10:55 2004 +0000
@@ -28,6 +28,7 @@
 ## contain the coefficients of the polynomial quotient and @var{r} will be
 ## a remander polynomial of lowest order.
 ## @end deftypefn
+##
 ## @seealso{conv, poly, roots, residue, polyval, polyderiv, and polyinteg}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/polynomial/polyderiv.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/polyderiv.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## Return the coefficients of the derivative of the polynomial whose
 ## coefficients are given by vector @var{c}.
 ## @end deftypefn
+##
 ## @seealso{poly, polyinteg, polyreduce, roots, conv, deconv, residue,
 ## filter, polyval, and polyvalm}
 

--- a/scripts/polynomial/polyinteg.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/polyinteg.m	Tue Oct 19 23:10:55 2004 +0000
@@ -24,6 +24,7 @@
 ##
 ## The constant of integration is set to zero.
 ## @end deftypefn
+##
 ## @seealso{poly, polyderiv, polyreduce, roots, conv, deconv, residue,
 ## filter, polyval, and polyvalm}
 

--- a/scripts/polynomial/polyout.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/polyout.m	Tue Oct 19 23:10:55 2004 +0000
@@ -33,6 +33,7 @@
 ##  @var{nargout} is zero).
 ##  @var{x} defaults to the string @code{"s"}.
 ## @end deftypefn
+##
 ## @seealso{polyval, polyvalm, poly, roots, conv, deconv, residue,
 ## filter, polyderiv, and polyinteg}
 

--- a/scripts/polynomial/polyreduce.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/polyreduce.m	Tue Oct 19 23:10:55 2004 +0000
@@ -22,6 +22,7 @@
 ## Reduces a polynomial coefficient vector to a minimum number of terms by
 ## stripping off any leading zeros.
 ## @end deftypefn
+##
 ## @seealso{poly, roots, conv, deconv, residue, filter, polyval,
 ## polyvalm, polyderiv, and polyinteg}
 

--- a/scripts/polynomial/polyval.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/polyval.m	Tue Oct 19 23:10:55 2004 +0000
@@ -27,6 +27,7 @@
 ## If @var{x} is a vector or matrix, the polynomial is evaluated at each of
 ## the elements of @var{x}.
 ## @end deftypefn
+##
 ## @seealso{polyvalm, poly, roots, conv, deconv, residue, filter,
 ## polyderiv, and polyinteg}
 

--- a/scripts/polynomial/polyvalm.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/polyvalm.m	Tue Oct 19 23:10:55 2004 +0000
@@ -27,6 +27,7 @@
 ##
 ## The argument @var{x} must be a square matrix.
 ## @end deftypefn
+##
 ## @seealso{polyval, poly, roots, conv, deconv, residue, filter,
 ## polyderiv, and polyinteg}
 

--- a/scripts/polynomial/residue.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/polynomial/residue.m	Tue Oct 19 23:10:55 2004 +0000
@@ -100,6 +100,7 @@
 ## @end example
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{poly, roots, conv, deconv, polyval, polyderiv, and polyinteg}
 
 ## Author: Tony Richardson <arichard@stark.cc.oh.us>

--- a/scripts/set/complement.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/set/complement.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{create_set, union, and intersection}
 
 ## Author: jwe

--- a/scripts/set/create_set.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/set/create_set.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{union, intersection, and complement}
 
 ## Author: jwe

--- a/scripts/set/intersection.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/set/intersection.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{create_set, union, and complement}
 
 ## Author: jwe

--- a/scripts/set/union.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/set/union.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## @end group
 ## @end example
 ## @end deftypefn
+##
 ## @seealso{create_set, intersection, and complement}
 
 ## Author: jwe

--- a/scripts/specfun/erfinv.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/specfun/erfinv.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Mapping Function} {} erfinv (@var{z})
 ## Computes the inverse of the error function.
 ## @end deftypefn
+##
 ## @seealso{erf and erfc}
 
 ## Author: KH <Kurt.Hornik@ci.tuwien.ac.at>

--- a/scripts/specfun/log2.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/specfun/log2.m	Tue Oct 19 23:10:55 2004 +0000
@@ -31,6 +31,7 @@
 ##  1/2 <= abs(f) < 1 and x = f * 2^e.
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{log, log10, logspace, and exp}
 
 ## Author: AW <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/specfun/pow2.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/specfun/pow2.m	Tue Oct 19 23:10:55 2004 +0000
@@ -39,6 +39,7 @@
 ##  f .* (2 .^ e).
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{nextpow2}
 
 ## Author: AW <Andreas.Weingessel@ci.tuwien.ac.at>

--- a/scripts/special-matrix/hankel.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/special-matrix/hankel.m	Tue Oct 19 23:10:55 2004 +0000
@@ -44,6 +44,7 @@
 ## @end example
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{vander, sylvester_matrix, hilb, invhilb, and toeplitz}
 
 ## Author: jwe

--- a/scripts/special-matrix/hilb.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/special-matrix/hilb.m	Tue Oct 19 23:10:55 2004 +0000
@@ -43,6 +43,7 @@
 ## @end example
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{hankel, vander, sylvester_matrix, invhilb, and toeplitz}
 
 ## Author: jwe

--- a/scripts/special-matrix/invhilb.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/special-matrix/invhilb.m	Tue Oct 19 23:10:55 2004 +0000
@@ -63,6 +63,7 @@
 ## finite precision of your computer's floating point arithmetic.
 ##
 ## @end deftypefn
+##
 ## @seealso{hankel, vander, sylvester_matrix, hilb, and toeplitz}
 
 ## Author: Dirk Laurie <dirk@siegfried.wisk.sun.ac.za>

--- a/scripts/special-matrix/sylvester_matrix.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/special-matrix/sylvester_matrix.m	Tue Oct 19 23:10:55 2004 +0000
@@ -29,6 +29,7 @@
 ## n = 2^k.
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{hankel, vander, hilb, invhilb, and toeplitz}
 
 ## Author: jwe

--- a/scripts/special-matrix/toeplitz.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/special-matrix/toeplitz.m	Tue Oct 19 23:10:55 2004 +0000
@@ -52,6 +52,7 @@
 ## @end example
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{hankel, vander, sylvester_matrix, hilb, and invhib}
 
 ## Author: jwe

--- a/scripts/special-matrix/vander.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/special-matrix/vander.m	Tue Oct 19 23:10:55 2004 +0000
@@ -46,6 +46,7 @@
 ## @end example
 ## @end ifinfo
 ## @end deftypefn
+##
 ## @seealso{hankel, sylvester_matrix, hilb, invhilb, and toeplitz}
 
 ## Author: jwe

--- a/scripts/statistics/base/median.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/statistics/base/median.m	Tue Oct 19 23:10:55 2004 +0000
@@ -43,6 +43,7 @@
 ## If @var{x} is a matrix, compute the median value for each
 ## column and return them in a row vector.
 ## @end deftypefn
+##
 ## @seealso{std and mean}
 
 ## Author: jwe

--- a/scripts/statistics/base/std.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/statistics/base/std.m	Tue Oct 19 23:10:55 2004 +0000
@@ -56,6 +56,7 @@
 ## The third argument @var{dim} determines the dimension along which the standard
 ## deviation is calculated.
 ## @end deftypefn
+##
 ## @seealso{mean and median}
 
 ## Author: jwe

--- a/scripts/strings/base2dec.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/strings/base2dec.m	Tue Oct 19 23:10:55 2004 +0000
@@ -42,6 +42,7 @@
 ## @end example
 ##
 ## @end deftypefn
+##
 ## @seealso{dec2base, dec2bin, bin2dec, hex2dec, dec2hex}
 
 ## Author: Daniel Calvelo <dcalvelo@yahoo.com>

--- a/scripts/strings/isletter.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/strings/isletter.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} isletter (@var{s})
 ## Returns true if @var{s} is a letter false otherwise.
 ## @end deftypefn
+##
 ## @seealso{isalpha}
 
 ## Author: jwe

--- a/scripts/strings/lower.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/strings/lower.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} lower (@var{s})
 ## Transform all letters in the string @var{s} to lower case.
 ## @end deftypefn
+##
 ## @seealso{tolower}
 
 ## Author: jwe

--- a/scripts/strings/upper.m	Tue Oct 19 18:40:48 2004 +0000
+++ b/scripts/strings/upper.m	Tue Oct 19 23:10:55 2004 +0000
@@ -21,6 +21,7 @@
 ## @deftypefn {Function File} {} upper (@var{s})
 ## Transform all letters in the string @var{s} to upper case.
 ## @end deftypefn
+##
 ## @seealso{toupper}
 
 ## Author: jwe