redo im_log_*mask() as classes

This commit is contained in:
John Cupitt 2013-10-20 16:10:22 +01:00
parent aa107b1bf7
commit 7ef4573f18
9 changed files with 351 additions and 277 deletions

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@ -1,5 +1,5 @@
19/10/13 started 7.37.0
- redone im_rotate_*mask45(), im_gauss_*mask*() as classes
- redone im_rotate_*mask45(), im_gauss_*mask*(), im_log_*mask*() as classes
18/10/13 started 7.36.3
- fix compiler warnings in ubuntu 13.10

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@ -3,7 +3,8 @@ noinst_LTLIBRARIES = libcreate.la
libcreate_la_SOURCES = \
create.c \
pcreate.h \
gauss.c \
gaussmat.c \
logmat.c \
buildlut.c \
invertlut.c \
tonelut.c \

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@ -111,7 +111,8 @@ void
vips_create_operation_init( void )
{
extern GType vips_black_get_type( void );
extern GType vips_gauss_get_type( void );
extern GType vips_gaussmat_get_type( void );
extern GType vips_logmat_get_type( void );
extern GType vips_gaussnoise_get_type( void );
#ifdef HAVE_PANGOFT2
extern GType vips_text_get_type( void );
@ -127,7 +128,8 @@ vips_create_operation_init( void )
extern GType vips_identity_get_type( void );
vips_black_get_type();
vips_gauss_get_type();
vips_gaussmat_get_type();
vips_logmat_get_type();
vips_gaussnoise_get_type();
#ifdef HAVE_PANGOFT2
vips_text_get_type();

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@ -13,7 +13,7 @@
* - set scale in _sep variant, why not
* 21/10/10
* - gtkdoc
* 20/10/10
* 20/10/13
* - redone as a class
*/
@ -62,7 +62,7 @@
#include "pcreate.h"
typedef struct _VipsGauss {
typedef struct _VipsGaussmat {
VipsCreate parent_instance;
double sigma;
@ -71,40 +71,38 @@ typedef struct _VipsGauss {
gboolean separable;
gboolean integer;
} VipsGauss;
} VipsGaussmat;
typedef struct _VipsGaussClass {
typedef struct _VipsGaussmatClass {
VipsCreateClass parent_class;
} VipsGaussClass;
} VipsGaussmatClass;
G_DEFINE_TYPE( VipsGauss, vips_gauss, VIPS_TYPE_CREATE );
G_DEFINE_TYPE( VipsGaussmat, vips_gaussmat, VIPS_TYPE_CREATE );
static int
vips_gauss_build( VipsObject *object )
vips_gaussmat_build( VipsObject *object )
{
VipsObjectClass *class = VIPS_OBJECT_GET_CLASS( object );
VipsCreate *create = VIPS_CREATE( object );
VipsGauss *gauss = (VipsGauss *) object;
VipsGaussmat *gaussmat = (VipsGaussmat *) object;
double sig2 = 2. * gaussmat->sigma * gaussmat->sigma;
int max_x = 8 * gaussmat->sigma > 5000 ? 5000 : 8 * gaussmat->sigma ;
int x, y;
int max_x;
int width, height;
double sig2; /* sig2 = 2. * sigma * sigma */
double sum;
if( VIPS_OBJECT_CLASS( vips_gauss_parent_class )->build( object ) )
if( VIPS_OBJECT_CLASS( vips_gaussmat_parent_class )->build( object ) )
return( -1 );
/* Find the size of the mask. Limit the mask size to 10k x 10k for
* sanity.
*/
sig2 = 2. * gauss->sigma * gauss->sigma;
max_x = 8 * gauss->sigma > 5000 ? 5000 : 8 * gauss->sigma ;
for( x = 0; x < max_x; x++ ) {
double v = exp( - ((double)(x * x)) / sig2 );
if( v < gauss->min_ampl )
if( v < gaussmat->min_ampl )
break;
}
if( x == max_x ) {
@ -112,7 +110,7 @@ vips_gauss_build( VipsObject *object )
return( -1 );
}
width = x * 2 + 1;
height = gauss->separable ? 1 : width;
height = gaussmat->separable ? 1 : width;
vips_image_init_fields( create->out,
width, height, 1,
@ -131,7 +129,7 @@ vips_gauss_build( VipsObject *object )
double distance = xo * xo + yo * yo;
double v = exp( -distance / sig2 );
if( gauss->integer )
if( gaussmat->integer )
v = VIPS_RINT( 20 * v );
*VIPS_MATRIX( create->out, x, y ) = v;
@ -146,7 +144,7 @@ vips_gauss_build( VipsObject *object )
}
static void
vips_gauss_class_init( VipsGaussClass *class )
vips_gaussmat_class_init( VipsGaussmatClass *class )
{
GObjectClass *gobject_class = G_OBJECT_CLASS( class );
VipsObjectClass *vobject_class = VIPS_OBJECT_CLASS( class );
@ -154,49 +152,49 @@ vips_gauss_class_init( VipsGaussClass *class )
gobject_class->set_property = vips_object_set_property;
gobject_class->get_property = vips_object_get_property;
vobject_class->nickname = "gauss";
vobject_class->nickname = "gaussmat";
vobject_class->description = _( "make a gaussian image" );
vobject_class->build = vips_gauss_build;
vobject_class->build = vips_gaussmat_build;
VIPS_ARG_DOUBLE( class, "sigma", 2,
_( "Radius" ),
_( "Radius of Gaussian" ),
VIPS_ARGUMENT_REQUIRED_INPUT,
G_STRUCT_OFFSET( VipsGauss, sigma ),
G_STRUCT_OFFSET( VipsGaussmat, sigma ),
0.000001, 10000.0, 1.0 );
VIPS_ARG_DOUBLE( class, "min_ampl", 3,
_( "Width" ),
_( "Minimum amplitude of Gaussian" ),
VIPS_ARGUMENT_REQUIRED_INPUT,
G_STRUCT_OFFSET( VipsGauss, min_ampl ),
G_STRUCT_OFFSET( VipsGaussmat, min_ampl ),
0.000001, 10000.0, 0.1 );
VIPS_ARG_BOOL( class, "separable", 4,
_( "Separable" ),
_( "Generate separable Gaussian" ),
VIPS_ARGUMENT_OPTIONAL_INPUT,
G_STRUCT_OFFSET( VipsGauss, separable ),
G_STRUCT_OFFSET( VipsGaussmat, separable ),
FALSE );
VIPS_ARG_BOOL( class, "integer", 5,
_( "Integer" ),
_( "Generate integer Gaussian" ),
VIPS_ARGUMENT_OPTIONAL_INPUT,
G_STRUCT_OFFSET( VipsGauss, integer ),
G_STRUCT_OFFSET( VipsGaussmat, integer ),
FALSE );
}
static void
vips_gauss_init( VipsGauss *gauss )
vips_gaussmat_init( VipsGaussmat *gaussmat )
{
gauss->sigma = 1;
gauss->min_ampl = 0.1;
gaussmat->sigma = 1;
gaussmat->min_ampl = 0.1;
}
/**
* vips_gauss:
* vips_gaussmat:
* @sigma: standard deviation of mask
* @min_ampl: minimum amplitude
* @...: %NULL-terminated list of optional named arguments
@ -231,13 +229,13 @@ vips_gauss_init( VipsGauss *gauss )
* Returns: 0 on success, -1 on error
*/
int
vips_gauss( VipsImage **out, double sigma, double min_ampl, ... )
vips_gaussmat( VipsImage **out, double sigma, double min_ampl, ... )
{
va_list ap;
int result;
va_start( ap, min_ampl );
result = vips_call_split( "gauss", ap, out, sigma, min_ampl );
result = vips_call_split( "gaussmat", ap, out, sigma, min_ampl );
va_end( ap );
return( result );

273
libvips/create/logmat.c Normal file
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@ -0,0 +1,273 @@
/* laplacian of logmatian
*
* Written on: 30/11/1989
* Updated on: 6/12/1991
* 7/8/96 JC
* - ansified, mem leaks plugged
* 20/11/98 JC
* - mask too large check added
* 26/3/02 JC
* - ahem, was broken since '96, thanks matt
* 16/7/03 JC
* - makes mask out to zero, not out to minimum, thanks again matt
* 22/10/10
* - gtkdoc
* 20/10/13
* - redone as a class from logmat.c
*/
/*
This file is part of VIPS.
VIPS is free software; you can redistribute it and/or modify
it under the terms of the GNU Lesser General Public License as published by
the Free Software Foundation; either version 2 of the License, or
(at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU Lesser General Public License for more details.
You should have received a copy of the GNU Lesser General Public License
along with this program; if not, write to the Free Software
Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA
02110-1301 USA
*/
/*
These files are distributed with VIPS - http://www.vips.ecs.soton.ac.uk
*/
/*
#define VIPS_DEBUG
*/
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif /*HAVE_CONFIG_H*/
#include <vips/intl.h>
#include <stdio.h>
#include <string.h>
#include <stdlib.h>
#include <math.h>
#include <vips/vips.h>
#include "pcreate.h"
typedef struct _VipsLogmat {
VipsCreate parent_instance;
double sigma;
double min_ampl;
gboolean separable;
gboolean integer;
} VipsLogmat;
typedef struct _VipsLogmatClass {
VipsCreateClass parent_class;
} VipsLogmatClass;
G_DEFINE_TYPE( VipsLogmat, vips_logmat, VIPS_TYPE_CREATE );
static int
vips_logmat_build( VipsObject *object )
{
VipsObjectClass *class = VIPS_OBJECT_GET_CLASS( object );
VipsCreate *create = VIPS_CREATE( object );
VipsLogmat *logmat = (VipsLogmat *) object;
double sig2 = logmat->sigma * logmat->sigma;
double last;
int x, y;
int width, height;
double sum;
if( VIPS_OBJECT_CLASS( vips_logmat_parent_class )->build( object ) )
return( -1 );
/* Find the size of the mask. We want to eval the mask out to the
* flat zero part, ie. beyond the minimum and to the point where it
* comes back up towards zero.
*/
last = 0.0;
for( x = 0; x < 5000; x++ ) {
const double distance = x * x;
double val;
/* Handbook of Pattern Recognition and image processing
* by Young and Fu AP 1986 pp 220-221
* temp = (1.0 / (2.0 * IM_PI * sig4)) *
(2.0 - (distance / sig2)) *
exp( (-1.0) * distance / (2.0 * sig2) )
.. use 0.5 to normalise
*/
val = 0.5 *
(2.0 - (distance / sig2)) *
exp( -distance / (2.0 * sig2) );
/* Stop when change in value (ie. difference from the last
* point) is positive (ie. we are going up) and absolute value
* is less than the min.
*/
if( val - last >= 0 &&
fabs( val ) < logmat->min_ampl )
break;
last = val;
}
if( x == 5000 ) {
vips_error( class->nickname, "%s", _( "mask too large" ) );
return( -1 );
}
width = x * 2 + 1;
height = logmat->separable ? 1 : width;
vips_image_init_fields( create->out,
width, height, 1,
VIPS_FORMAT_DOUBLE, VIPS_CODING_NONE, VIPS_INTERPRETATION_B_W,
1.0, 1.0 );
vips_demand_hint( create->out,
VIPS_DEMAND_STYLE_ANY, NULL );
if( vips_image_write_prepare( create->out ) )
return( -1 );
sum = 0.0;
for( y = 0; y < height; y++ ) {
for( x = 0; x < width; x++ ) {
int xo = x - width / 2;
int yo = y - height / 2;
double distance = xo * xo + yo * yo;
double v = 0.5 *
(2.0 - (distance / sig2)) *
exp( -distance / (2.0 * sig2) );
if( logmat->integer )
v = VIPS_RINT( 20 * v );
*VIPS_MATRIX( create->out, x, y ) = v;
sum += v;
}
}
vips_image_set_double( create->out, "scale", sum );
vips_image_set_double( create->out, "offset", 0.0 );
return( 0 );
}
static void
vips_logmat_class_init( VipsLogmatClass *class )
{
GObjectClass *gobject_class = G_OBJECT_CLASS( class );
VipsObjectClass *vobject_class = VIPS_OBJECT_CLASS( class );
gobject_class->set_property = vips_object_set_property;
gobject_class->get_property = vips_object_get_property;
vobject_class->nickname = "logmat";
vobject_class->description = _( "make a laplacian of gaussian image" );
vobject_class->build = vips_logmat_build;
VIPS_ARG_DOUBLE( class, "sigma", 2,
_( "Radius" ),
_( "Radius of Logmatian" ),
VIPS_ARGUMENT_REQUIRED_INPUT,
G_STRUCT_OFFSET( VipsLogmat, sigma ),
0.000001, 10000.0, 1.0 );
VIPS_ARG_DOUBLE( class, "min_ampl", 3,
_( "Width" ),
_( "Minimum amplitude of Logmatian" ),
VIPS_ARGUMENT_REQUIRED_INPUT,
G_STRUCT_OFFSET( VipsLogmat, min_ampl ),
0.000001, 10000.0, 0.1 );
VIPS_ARG_BOOL( class, "separable", 4,
_( "Separable" ),
_( "Generate separable Logmatian" ),
VIPS_ARGUMENT_OPTIONAL_INPUT,
G_STRUCT_OFFSET( VipsLogmat, separable ),
FALSE );
VIPS_ARG_BOOL( class, "integer", 5,
_( "Integer" ),
_( "Generate integer Logmatian" ),
VIPS_ARGUMENT_OPTIONAL_INPUT,
G_STRUCT_OFFSET( VipsLogmat, integer ),
FALSE );
}
static void
vips_logmat_init( VipsLogmat *logmat )
{
logmat->sigma = 1;
logmat->min_ampl = 0.1;
}
/**
* vips_logmat:
* @sigma: standard deviation of mask
* @min_ampl: minimum amplitude
* @...: %NULL-terminated list of optional named arguments
*
* Optional arguments:
*
* @separable: generate a separable logmatian
* @integer: generate an integer logmatian
*
* Creates a circularly symmetric Laplacian of Gaussian mask
* of radius
* @sigma. The size of the mask is determined by the variable @min_ampl;
* if for instance the value .1 is entered this means that the produced mask
* is clipped at values within 10 persent of zero, and where the change
* between mask elements is less than 10%.
*
* The program uses the following equation: (from Handbook of Pattern
* Recognition and image processing by Young and Fu, AP 1986 pages 220-221):
*
* H(r) = (1 / (2 * M_PI * s4)) *
* (2 - (r2 / s2)) *
* exp(-r2 / (2 * s2))
*
* where s2 = @sigma * @sigma, s4 = s2 * s2, r2 = r * r.
*
* The generated mask has odd size and its maximum value is normalised to
* 1.0, unless @integer is set.
*
* If @separable is set, only the centre horizontal is generated. This is
* useful for separable convolutions.
*
* If @integer is set, an integer logmatian is generated. This is useful for
* integer convolutions.
*
* "scale" is set to the sum of all the mask elements.
*
* See also: vips_gauss(), vips_conv().
*
* Returns: 0 on success, -1 on error
*/
int
vips_logmat( VipsImage **out, double sigma, double min_ampl, ... )
{
va_list ap;
int result;
va_start( ap, min_ampl );
result = vips_call_split( "logmat", ap, out, sigma, min_ampl );
va_end( ap );
return( result );
}

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@ -45,7 +45,6 @@ libdeprecated_la_SOURCES = \
im_mask2vips.c \
im_vips2mask.c \
rotmask.c \
im_logmasks.c \
rw_mask.c \
im_matcat.c \
im_matinv.c \

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@ -1,238 +0,0 @@
/* laplacian of gaussian
*
* Written on: 30/11/1989
* Updated on: 6/12/1991
* 7/8/96 JC
* - ansified, mem leaks plugged
* 20/11/98 JC
* - mask too large check added
* 26/3/02 JC
* - ahem, was broken since '96, thanks matt
* 16/7/03 JC
* - makes mask out to zero, not out to minimum, thanks again matt
* 22/10/10
* - gtkdoc
*/
/*
This file is part of VIPS.
VIPS is free software; you can redistribute it and/or modify
it under the terms of the GNU Lesser General Public License as published by
the Free Software Foundation; either version 2 of the License, or
(at your option) any later version.
This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU Lesser General Public License for more details.
You should have received a copy of the GNU Lesser General Public License
along with this program; if not, write to the Free Software
Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA
02110-1301 USA
*/
/*
These files are distributed with VIPS - http://www.vips.ecs.soton.ac.uk
*/
/*
#define PIM_RINT 1
*/
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif /*HAVE_CONFIG_H*/
#include <vips/intl.h>
#include <stdio.h>
#include <math.h>
#include <vips/vips.h>
#include <vips/util.h>
#define IM_MAXMASK 256
/**
* im_log_dmask:
* @filename: the returned mask has this set as the filename
* @sigma: standard deviation of mask
* @min_ampl: minimum amplitude
*
* im_log_dmask() creates a circularly symmetric Laplacian of Gaussian mask
* of radius
* @sigma. The size of the mask is determined by the variable @min_ampl;
* if for instance the value .1 is entered this means that the produced mask
* is clipped at values within 10 persent of zero, and where the change
* between mask elements is less than 10%.
*
* The program uses the following equation: (from Handbook of Pattern
* Recognition and image processing by Young and Fu, AP 1986 pages 220-221):
*
* H(r) = (1 / (2 * M_PI * s4)) *
* (2 - (r2 / s2)) *
* exp(-r2 / (2 * s2))
*
* where s2 = sigma * sigma, s4 = s2 * s2, r2 = r * r.
*
* The generated mask has odd size and its maximum value is normalised to 1.0.
*
* See also: im_log_imask(), im_gauss_dmask(), im_conv().
*
* Returns: the calculated mask on success, or NULL on error.
*/
DOUBLEMASK *
im_log_dmask( const char *filename, double sigma, double min_ampl )
{
const double sig2 = sigma * sigma;
double last;
int x, y, k;
double *pt1, *pt2, *pt3, *pt4;
int xm, ym;
int xm2, ym2; /* xm2 = xm/2 */
int offset;
double *cf, *cfs, *mc;
DOUBLEMASK *m;
double sum;
/* Find the size of the mask depending on the entered data. We want to
* eval the mask out to the flat zero part, ie. beyond the minimum and
* to the point where it comes back up towards zero.
*/
last = 0.0;
for( x = 0; x < IM_MAXMASK; x++ ) {
const double distance = x * x;
double val;
/* Handbook of Pattern Recognition and image processing
* by Young and Fu AP 1986 pp 220-221
* temp = (1.0 / (2.0 * IM_PI * sig4)) *
(2.0 - (distance / sig2)) *
exp( (-1.0) * distance / (2.0 * sig2) )
.. use 0.5 to normalise
*/
val = 0.5 *
(2.0 - (distance / sig2)) *
exp( -distance / (2.0 * sig2) );
/* Stop when change in value (ie. difference from the last
* point) is positive (ie. we are going up) and absolute value
* is less than the min.
*/
if( val - last >= 0 &&
fabs( val ) < min_ampl )
break;
last = val;
}
if( x == IM_MAXMASK ) {
im_error( "im_log_dmask", "%s", _( "mask too large" ) );
return( NULL );
}
xm2 = x;
ym2 = x;
xm = xm2 * 2 + 1;
ym = ym2 * 2 + 1;
if( !(cfs = IM_ARRAY( NULL, (xm2 + 1) * (ym2 + 1), double )) )
return( NULL );
/* Make 1/4 of the mask.
*/
for( k = 0, y = 0; y <= ym2; y++ )
for( x = 0; x <= xm2; x++, k++ ) {
const double distance = x * x + y * y;
cfs[k] = 0.5 *
(2.0 - (distance / sig2)) *
exp( -distance / (2.0 * sig2) );
}
#ifdef PIM_RINT
for( k = 0, y = 0; y <= ym2; y++ ) {
for( x = 0; x <= xm2; x++, k++ )
fprintf( stderr, "%3.2f ", cfs[k] );
fprintf( stderr, "\n" );
}
#endif
if( !(m = im_create_dmask( filename, xm, ym )) ) {
im_free( cfs );
return( NULL );
}
/* Copy the 1/4 cfs into the m
*/
cf = cfs;
offset = xm2 * (xm + 1);
mc = m->coeff + offset;
for( y = 0; y <= ym2; y++ ) {
for( x = 0; x <= xm2; x++ ) {
pt1 = mc + (y * xm) + x;
pt2 = mc - (y * xm) + x;
pt3 = mc + (y * xm) - x;
pt4 = mc - (y * xm) - x;
*pt1 = cf[x];
*pt2 = cf[x];
*pt3 = cf[x];
*pt4 = cf[x];
}
cf += (xm2 + 1);
}
im_free( cfs );
sum = 0.0;
for( k = 0, y = 0; y < m->ysize; y++ )
for( x = 0; x < m->xsize; x++, k++ )
sum += m->coeff[k];
m->scale = sum;
m->offset = 0.0;
#ifdef PIM_RINT
im_print_dmask( m );
#endif
return( m );
}
/**
* im_log_imask:
* @filename: the returned mask has this set as the filename
* @sigma: standard deviation of mask
* @min_ampl: minimum amplitude
*
* im_log_imask() works exactly as im_log_dmask(), but the returned mask
* is scaled so that it's maximum value it set to 100.
*
* See also: im_log_dmask(), im_gauss_imask(), im_conv().
*
* Returns: the calculated mask on success, or NULL on error.
*/
INTMASK *
im_log_imask( const char *filename, double sigma, double min_ampl )
{
DOUBLEMASK *dm;
INTMASK *im;
if( !(dm = im_log_dmask( filename, sigma, min_ampl )) )
return( NULL );
if( !(im = im_scale_dmask( dm, dm->filename )) ) {
im_free_dmask( dm );
return( NULL );
}
im_free_dmask( dm );
return( im ) ;
}

View File

@ -1900,7 +1900,7 @@ im_gauss_dmask( const char *filename, double sigma, double min_ampl )
VipsImage *t;
DOUBLEMASK *msk;
if( vips_gauss( &t, sigma, min_ampl,
if( vips_gaussmat( &t, sigma, min_ampl,
NULL ) )
return( NULL );
if( !(msk = im_vips2mask( t, filename )) ) {
@ -1918,7 +1918,7 @@ im_gauss_dmask_sep( const char *filename, double sigma, double min_ampl )
VipsImage *t;
DOUBLEMASK *msk;
if( vips_gauss( &t, sigma, min_ampl,
if( vips_gaussmat( &t, sigma, min_ampl,
"seperable", TRUE,
NULL ) )
return( NULL );
@ -1937,7 +1937,7 @@ im_gauss_imask( const char *filename, double sigma, double min_ampl )
VipsImage *t;
INTMASK *msk;
if( vips_gauss( &t, sigma, min_ampl,
if( vips_gaussmat( &t, sigma, min_ampl,
"integer", TRUE,
NULL ) )
return( NULL );
@ -1956,7 +1956,7 @@ im_gauss_imask_sep( const char *filename, double sigma, double min_ampl )
VipsImage *t;
INTMASK *msk;
if( vips_gauss( &t, sigma, min_ampl,
if( vips_gaussmat( &t, sigma, min_ampl,
"integer", TRUE,
"seperable", TRUE,
NULL ) )
@ -1970,6 +1970,43 @@ im_gauss_imask_sep( const char *filename, double sigma, double min_ampl )
return( msk );
}
INTMASK *
im_log_imask( const char *filename, double sigma, double min_ampl )
{
VipsImage *t;
INTMASK *msk;
if( vips_logmat( &t, sigma, min_ampl,
"integer", TRUE,
NULL ) )
return( NULL );
if( !(msk = im_vips2imask( t, filename )) ) {
g_object_unref( t );
return( NULL );
}
g_object_unref( t );
return( msk );
}
DOUBLEMASK *
im_log_dmask( const char *filename, double sigma, double min_ampl )
{
VipsImage *t;
DOUBLEMASK *msk;
if( vips_logmat( &t, sigma, min_ampl,
NULL ) )
return( NULL );
if( !(msk = im_vips2mask( t, filename )) ) {
g_object_unref( t );
return( NULL );
}
g_object_unref( t );
return( msk );
}
int
im_recomb( IMAGE *in, IMAGE *out, DOUBLEMASK *recomb )
{

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@ -47,7 +47,9 @@ int vips_xyz( VipsImage **out, int width, int height, ... )
__attribute__((sentinel));
int vips_grey( VipsImage **out, int width, int height, ... )
__attribute__((sentinel));
int vips_gauss( VipsImage **out, double sigma, double min_ampl, ... )
int vips_gaussmat( VipsImage **out, double sigma, double min_ampl, ... )
__attribute__((sentinel));
int vips_logmat( VipsImage **out, double sigma, double min_ampl, ... )
__attribute__((sentinel));
int vips_text( VipsImage **out, const char *text, ... )