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/* $Id: fors_extract.c,v 1.45 2011-10-13 14:29:24 cgarcia Exp $
*
* This file is part of the FORS Library
* Copyright (C) 2002-2010 European Southern Observatory
*
* This program is free software; you can redistribute it and/or modify
* it under the terms of the GNU General Public License as published by
* the Free Software Foundation; either version 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 General Public License for more details.
*
* You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software
* Foundation, Inc., 51 Franklin St, Fifth Floor, Boston, MA 02110-1301 USA
*/
/*
* $Author: cgarcia $
* $Date: 2011-10-13 14:29:24 $
* $Revision: 1.45 $
* $Name: not supported by cvs2svn $
*/
#ifdef HAVE_CONFIG_H
#include <config.h>
#endif
#include <fors_extract.h>
#include <fors_star.h>
#include <fors_tools.h>
#include <fors_dfs.h>
#include <fors_pfits.h>
#include <fors_utils.h>
#include <cpl.h>
#include <string.h>
#include <stdbool.h>
#include <math.h>
/**
* @defgroup fors_extract Image source extraction
*/
/**@{*/
/*-----------------------------------------------------------------------------
(Proto)types
-----------------------------------------------------------------------------*/
struct _extract_method
{
enum {SEX, TEST} method;
const char *sex_exe;
const char *sex_config;
const char *sex_mag;
const char *sex_magerr;
int sex_radius;
};
static fors_star_list *
extract_sex( const fors_image *image,
const fors_setting *setting,
const char *sex_exe,
const char *sex_config,
const char *sex_mag,
const char *sex_magerr,
int radius,
double magsyserr,
fors_extract_sky_stats *sky_stats,
cpl_image **background,
cpl_table **extracted_sources);
static fors_star_list *
extract_test( fors_extract_sky_stats *sky_stats,
cpl_image **background,
cpl_table **extracted_sources);
/*-----------------------------------------------------------------------------
Implementation
-----------------------------------------------------------------------------*/
/*----------------------------------------------------------------------------*/
/**
* @brief Check SExtractor object feature: FLAG
* @param SExtractor object's binary contamination flags
* @return 1 if successful, 0 on failure
*
* All FLAGS 1, 2, 4, ..., 128 are severe enough that
* we do not want to use the source for photometry
* see SExtractor doc. for the meaning of each flag.
*/
/*----------------------------------------------------------------------------*/
bool
fors_extract_check_sex_flag( unsigned int sex_flag)
{
return (sex_flag == 0x0);
}
/*----------------------------------------------------------------------------*/
/**
* @brief Check a sextracted star for validity
* @param star (S)Extracted star
* @param ref_img (Optional) reference image (to check for image range)
* @return 1 if successful, 0 on failure
*
* The following SExtractor failures are caught:
* - Check for allowed general parameters using fors_star_check_values()
* - Invalid SExtractor magnitude (can be 99.0)
* - (x, y) out of range (if @a ref_img != NULL)
*
* @todo
* - FIXME: FAP: verify the criterion for magnitude rejection
*/
/*----------------------------------------------------------------------------*/
bool
fors_extract_check_sex_star( const fors_star *star,
const cpl_image *ref_img)
{
bool success = 1;
if (star == NULL)
return 0;
success &= fors_star_check_values(star);
success &= (star->magnitude < 98);
if (ref_img != NULL)
{
success &= star->pixel->x >= 1;
success &= star->pixel->x <= cpl_image_get_size_x(ref_img);
success &= star->pixel->y >= 1;
success &= star->pixel->y <= cpl_image_get_size_y(ref_img);
}
return success;
}
/*----------------------------------------------------------------------------*/
/**
* @brief Define recipe parameters
* @param parameters parameter list to fill
* @param context parameters context
*/
/*----------------------------------------------------------------------------*/
void
fors_extract_define_parameters( cpl_parameterlist *parameters,
const char *context)
{
cpl_parameter *p;
const char *full_name = NULL;
const char *name;
/*
name = "extract_method";
full_name = cpl_sprintf("%s.%s", context, name);
p = cpl_parameter_new_enum(full_name,
CPL_TYPE_STRING,
"Source extraction method",
context,
"sex", 2,
"sex", "test");
cpl_parameter_set_alias(p, CPL_PARAMETER_MODE_CLI, name);
cpl_parameter_disable(p, CPL_PARAMETER_MODE_ENV);
cpl_parameterlist_append(parameters, p);
cpl_free((void *)full_name);
*/
name = "sex_exe";
full_name = cpl_sprintf("%s.%s", context, name);
p = cpl_parameter_new_value(full_name,
CPL_TYPE_STRING,
"SExtractor executable",
context,
FORS_SEXTRACTOR_PATH "/sex");
cpl_parameter_set_alias(p, CPL_PARAMETER_MODE_CLI, name);
cpl_parameter_disable(p, CPL_PARAMETER_MODE_ENV);
cpl_parameterlist_append(parameters, p);
cpl_free((void *)full_name);
name = "sex_config";
full_name = cpl_sprintf("%s.%s", context, name);
p = cpl_parameter_new_value(full_name,
CPL_TYPE_STRING,
"SExtractor configuration file",
context,
FORS_SEXTRACTOR_CONFIG "/fors.sex");
cpl_parameter_set_alias(p, CPL_PARAMETER_MODE_CLI, name);
cpl_parameter_disable(p, CPL_PARAMETER_MODE_ENV);
cpl_parameterlist_append(parameters, p);
cpl_free((void *)full_name);
name = "sex_mag";
full_name = cpl_sprintf("%s.%s", context, name);
p = cpl_parameter_new_value(full_name,
CPL_TYPE_STRING,
"SExtractor magnitude",
context,
"MAG_APER");
cpl_parameter_set_alias(p, CPL_PARAMETER_MODE_CLI, name);
cpl_parameter_disable(p, CPL_PARAMETER_MODE_ENV);
cpl_parameterlist_append(parameters, p);
cpl_free((void *)full_name);
name = "sex_magerr";
full_name = cpl_sprintf("%s.%s", context, name);
p = cpl_parameter_new_value(full_name,
CPL_TYPE_STRING,
"SExtractor magnitude error",
context,
"MAGERR_APER");
cpl_parameter_set_alias(p, CPL_PARAMETER_MODE_CLI, name);
cpl_parameter_disable(p, CPL_PARAMETER_MODE_ENV);
cpl_parameterlist_append(parameters, p);
cpl_free((void *)full_name);
name = "sex_radius";
full_name = cpl_sprintf("%s.%s", context, name);
p = cpl_parameter_new_value(full_name,
CPL_TYPE_INT,
"Background error map median filter "
"radius (unbinned pixels)",
context,
64);
cpl_parameter_set_alias(p, CPL_PARAMETER_MODE_CLI, name);
cpl_parameter_disable(p, CPL_PARAMETER_MODE_ENV);
cpl_parameterlist_append(parameters, p);
cpl_free((void *)full_name); full_name = NULL;
return;
}
/*----------------------------------------------------------------------------*/
#undef cleanup
#define cleanup \
do { \
cpl_free((void *)name); \
cpl_free((void *)method); \
} while (0)
/**
* @brief Get extraction method from parameter list
* @param parameters recipe parameter list
* @param context read extraction method from this context
* @return newly allocated extraction method
*
* The parameter list should have been previously created using
* fors_extract_define_parameters()
*/
/*----------------------------------------------------------------------------*/
extract_method *
fors_extract_method_new( const cpl_parameterlist *parameters,
const char *context)
{
extract_method *em = cpl_malloc(sizeof(*em));
const char *name = NULL;
const char *method = NULL;
cpl_msg_info(cpl_func, "Extraction method:");
cpl_msg_indent_more();
//"sex" method is the default. The parameter won't appear when calling
//the recipe from esorex, but it will in the unit tests fors_zeropoint-test,
//fors_img_science-test.
name = cpl_sprintf("%s.%s", context, "extract_method");
if(cpl_parameterlist_find_const(parameters, name) == NULL)
method = cpl_sprintf("%s", "sex");
else
method = cpl_sprintf("%s",dfs_get_parameter_string_const(parameters, name));
cpl_free((void *)name); name = NULL;
cpl_msg_indent_less();
assure( !cpl_error_get_code(), return NULL, NULL );
assure( method != NULL, return NULL, NULL );
if (strcmp(method, "sex") == 0) {
em->method = SEX;
cpl_msg_indent_more();
name = cpl_sprintf("%s.%s", context, "sex_exe");
em->sex_exe = dfs_get_parameter_string_const(parameters,
name);
cpl_free((void *)name); name = NULL;
cpl_msg_indent_less();
cpl_msg_indent_more();
name = cpl_sprintf("%s.%s", context, "sex_config");
em->sex_config = dfs_get_parameter_string_const(parameters,
name);
cpl_free((void *)name); name = NULL;
cpl_msg_indent_less();
cpl_msg_indent_more();
name = cpl_sprintf("%s.%s", context, "sex_mag");
em->sex_mag = dfs_get_parameter_string_const(parameters,
name);
cpl_free((void *)name); name = NULL;
cpl_msg_indent_less();
cpl_msg_indent_more();
name = cpl_sprintf("%s.%s", context, "sex_magerr");
em->sex_magerr = dfs_get_parameter_string_const(parameters,
name);
cpl_free((void *)name); name = NULL;
cpl_msg_indent_less();
cpl_msg_indent_more();
name = cpl_sprintf("%s.%s", context, "sex_radius");
em->sex_radius = dfs_get_parameter_int_const(parameters,
name);
cpl_free((void *)name); name = NULL;
cpl_msg_indent_less();
}
else if (strcmp(method, "test") == 0) {
em->method = TEST;
}
else {
assure( false, return NULL, "Unknown extraction method '%s'", method);
}
cleanup;
return em;
}
/*----------------------------------------------------------------------------*/
/**
* @brief Deallocate extraction method and set the pointer to NULL
*/
/*----------------------------------------------------------------------------*/
void
fors_extract_method_delete( extract_method **em)
{
if (em && *em) {
cpl_free(*em); *em = NULL;
}
return;
}
/*----------------------------------------------------------------------------*/
#undef cleanup
#define cleanup
/**
* @brief Extract sources
* @param image source image
* @param setting instrument setting (gain)
* @param em extraction method to use
* @param sky_stats (output) statistics on determined sky
* @param background (output) inferred background image
* @param extracted_sources (output) if non-NULL, table of extracted sources
* @return newly allocated list of extracted stars
*/
/*----------------------------------------------------------------------------*/
fors_star_list *
fors_extract( const fors_image *image,
const fors_setting *setting,
const extract_method *em,
double magsyserr,
fors_extract_sky_stats *sky_stats,
cpl_image **background,
cpl_table **extracted_sources)
{
assure( em != NULL, return NULL, NULL );
cpl_msg_info(cpl_func, "Extracting sources");
switch (em->method ) {
case SEX: return extract_sex(image, setting,
em->sex_exe,
em->sex_config,
em->sex_mag,
em->sex_magerr,
em->sex_radius,
magsyserr,
sky_stats,
background,
extracted_sources); break;
case TEST: return extract_test(sky_stats, background, extracted_sources); break;
default:
assure( false, return NULL, "Unknown method %d", em->method );
break;
}
}
/*----------------------------------------------------------------------------*/
#undef cleanup
#define cleanup \
do { \
cpl_table_delete(out); out = NULL; \
cpl_free((void *)command); \
cpl_image_delete(work_back); work_back = NULL; \
cpl_image_delete(bmaxsigma); bmaxsigma = NULL; \
cpl_image_delete(bsigma); bsigma = NULL; \
fors_image_delete(&fbsigma); \
} while (0)
/**
* @brief Extract sources using SExtractor
* @param image source image
* @param setting instrument setting (gain)
* @param sex_exe SExtractor executable
* @param sex_config SExtractor configuration file
* @param sex_mag SExtractor catalog magnitude
* @param sex_magerr SExtractor catalog magnitude error
* @param radius background error map median filter radius
* @param sky_stats (output) statistics on determined sky
* @param background (output) background image
* @param extracted_sources (output) if non-NULL, SExtractor output table
* @return newly allocated list of stars
*
* Note: The gain given in the setting must describe the
* image. Therefore, if the provided value of the gain is just
* the detector gain, the input image must not be stacked or
* normalized to e.g. 1s exposure time.
*
* A background error map is given to SExtractor. This error map is
* obtained by applying a median filter to the input image error map
* (in order to remove sources).
*/
/*----------------------------------------------------------------------------*/
static fors_star_list *
extract_sex( const fors_image *image,
const fors_setting *setting,
const char *sex_exe,
const char *sex_config,
const char *sex_mag,
const char *sex_magerr,
int radius,
double magsyserr,
fors_extract_sky_stats *sky_stats,
cpl_image **background,
cpl_table **extracted_sources)
{
const char *const filename_data = "sextract_data.fits";
const char *const filename_sigma = "sextract_bkg_sigma.fits";
const char *const filename_cat = "sextract_cat.fits";
const char *const filename_bkg = "sextract_bkg.fits";
cpl_table *out = NULL;
const char *command = NULL;
fors_star_list *stars = NULL;
cpl_image *work_back = NULL;
cpl_image *bmaxsigma = NULL;
cpl_image *bsigma = NULL;
fors_image *fbsigma = NULL;
fors_image *cropped = NULL;
int croplx, croply, cropux, cropuy;
const char *const filename_data_full = "sextract_data_full.fits";
const char *const filename_sigma_full = "sextract_bkg_sigma_full.fits";
int vignetted = 1;
assure( setting != NULL, return NULL, NULL );
assure( image != NULL, return NULL, NULL );
assure( sky_stats != NULL, return NULL, NULL );
assure( background != NULL, return NULL, NULL );
/*
* In case of new chips, crop
*/
if (strcmp(setting->chip_id, "CCID20-14-5-6") == 0) {
croplx = 380 / setting->binx;
croply = 626 / setting->biny;
cropux = 3714 / setting->binx;
cropuy = 2048 / setting->biny;
}
else if (strcmp(setting->chip_id, "CCID20-14-5-3") == 0) {
croplx = 380 / setting->binx;
croply = 2 / setting->biny;
cropux = 3714 / setting->binx;
cropuy = 1920 / setting->biny;
}
else if (strncmp(setting->chip_id, "Marl", 4) == 0) {
croplx = 380 / setting->binx;
croply = 694 / setting->biny;
cropux = 3690 / setting->binx;
cropuy = 2048 / setting->biny;
}
else if (strncmp(setting->chip_id, "Norm", 4) == 0) {
croplx = 380 / setting->binx;
croply = 2 / setting->biny;
cropux = 3690 / setting->binx;
cropuy = 1894 / setting->biny;
}
else {
vignetted = 0;
}
cropped = (fors_image *)image; /* As a default.... */
if (vignetted) {
fors_image_save_sex(image, NULL,
filename_data_full,
filename_sigma_full,
radius);
assure( !cpl_error_get_code(), return NULL,
"Could not save image to %s and %s",
filename_data_full, filename_sigma_full);
cropped = fors_image_duplicate(image);
fors_image_crop(cropped, croplx, croply, cropux, cropuy);
}
/* provide data and error bars in separate files,
pass to sextractor */
fors_image_save_sex(cropped, NULL,
filename_data,
filename_sigma,
radius);
assure( !cpl_error_get_code(), return NULL,
"Could not save image to %s and %s",
filename_data, filename_sigma);
if (vignetted)
fors_image_delete(&cropped);
/*
* A = load filename_sigma
*
* M = fors_image_max_filter(A)
*
* |A-M|
*/
command = cpl_sprintf("%s %s,%s "
"-c %s "
/* Use SExtractor's double mode which is probably
more tested and more bugfree than the
single image mode */
"-GAIN %f " /* Different terminology here:
SExtractor-gain == ESO-conad,
unit = e- / ADU
*/
"-PIXEL_SCALE %f "
"-CHECKIMAGE_TYPE BACKGROUND "
"-CHECKIMAGE_NAME %s "
"-WEIGHT_TYPE MAP_RMS "
"-WEIGHT_IMAGE %s,%s "
"-CATALOG_TYPE FITS_1.0 "
"-CATALOG_NAME %s",
sex_exe,
filename_data, filename_data,
sex_config,
1.0/setting->average_gain,
setting->pixel_scale,
filename_bkg,
filename_sigma, filename_sigma,
filename_cat);
cpl_msg_info(cpl_func, "Running '%s'", command);
assure( system(command) == 0, return stars, "'%s' failed", command);
/*
* The background map is here used just to evaluate a QC parameter,
* and is also returned to the caller.
*/
{
int plane = 0;
int extension = 0;
*background = cpl_image_load(filename_bkg,
CPL_TYPE_FLOAT, plane, extension);
assure( !cpl_error_get_code(), return NULL,
"Could not load SExtractor background image %s",
filename_bkg );
if (vignetted) {
work_back = cpl_image_new(fors_image_get_size_x(image),
fors_image_get_size_y(image),
CPL_TYPE_FLOAT);
cpl_image_copy(work_back, *background, croplx, croply);
assure( !cpl_error_get_code(), return NULL,
"Could not insert background image %s",
filename_bkg );
cpl_image_delete(*background);
*background = work_back;
work_back = NULL;
}
/*
* To avoid using the non-illuminated parts, use only the central
* 100x100 window.
*
* It does not make too much sense to trend these QC parameters
* anyway because they mostly describe the individual science
* exposures.
*/
int nx = cpl_image_get_size_x(*background);
int ny = cpl_image_get_size_y(*background);
int xlo = nx/2 - 50;
int xhi = nx/2 + 50;
int ylo = ny/2 - 50;
int yhi = ny/2 + 50;
if (xlo < 0) xlo = 0; /* Just in case... */
if (xhi >= nx) xhi = nx - 1;
if (ylo < 0) ylo = 0;
if (yhi >= ny) yhi = ny - 1;
work_back = cpl_image_duplicate(*background);
sky_stats->mean = cpl_image_get_mean_window(work_back,
xlo, ylo, xhi, yhi);
sky_stats->median = cpl_image_get_median_window(work_back,
xlo, ylo, xhi, yhi);
cpl_image_subtract_scalar(work_back, sky_stats->median);
cpl_image_abs(work_back);
sky_stats->rms = cpl_image_get_median_window(work_back,
xlo, ylo, xhi, yhi)
* STDEV_PR_MAD;
cpl_image_delete(work_back); work_back = NULL;
assure( !cpl_error_get_code(), return NULL,
"Could not calculate sky statistics" );
}
cpl_msg_info(cpl_func, "Background = %f +- %f ADU",
sky_stats->median, sky_stats->rms);
/*
* SExtractors background estimation is not reliable near
* non-illuminated areas. The underestimated background
* leads to false detections.
* Therefore, reject sources which are too close to the
* illumination edge. The edge is masked using a max filter
* on the smoothed variance image of the background map.
* The filter must have comparable size to the SExtractor
* BACK_SIZE parameter. The discrimination level is half-way
* between the high-variance and low-variance regions.
*/
float level;
{
int xradius = 64;
int yradius = 64;
int plane = 0;
int extension = 0;
if (vignetted) {
bsigma = cpl_image_load(filename_sigma_full,
CPL_TYPE_FLOAT, plane, extension);
}
else {
bsigma = cpl_image_load(filename_sigma,
CPL_TYPE_FLOAT, plane, extension);
}
assure( !cpl_error_get_code(), return NULL,
"Could not load SExtractor background error image %s",
filename_sigma );
/*
* Duplication is necessary for creating the fors_image
* to be passed to fors_image_filter_max_create()
*/
/* this wraps the fors_image around the cpl images,
* so set them to NULL */
fbsigma = fors_image_new(cpl_image_duplicate(bsigma), bsigma);
bsigma = NULL;
{
bool use_variance = true;
bmaxsigma = fors_image_filter_max_create(fbsigma, xradius,
yradius, use_variance);
/* cpl_image_save(bmaxsigma, "/tmp/test.fits", CPL_BPP_IEEE_FLOAT, NULL,
CPL_IO_DEFAULT); */
}
fors_image_delete(&fbsigma);
/*
This is not robust if there are no non-illuminated areas.
maxima = cpl_image_get_max(bmaxsigma);
minima = cpl_image_get_min(bmaxsigma);
level = (maxima + minima) / 2;
*/
/* 5 sigma rejection */
level = cpl_image_get_median(bmaxsigma) * 5;
cpl_msg_debug(cpl_func, "Threshold level = %f",
level);
}
out = cpl_table_load(filename_cat, 1, 1);
assure( !cpl_error_get_code(), return NULL,
"Could not load SExtractor output table %s",
filename_cat);
/* Validate sextractor output */
assure( cpl_table_has_column(out, "FLAGS"), return NULL,
"%s: Missing column: %s", filename_cat, "FLAGS");
assure( cpl_table_has_column(out, "CLASS_STAR"), return NULL,
"%s: Missing column: %s", filename_cat, "CLASS_STAR");
assure( cpl_table_has_column(out, "BACKGROUND"), return NULL,
"%s: Missing column: %s", filename_cat, "BACKGROUND");
assure( cpl_table_has_column(out, "X_IMAGE"), return NULL,
"%s: Missing column: %s", filename_cat, "X_IMAGE");
assure( cpl_table_has_column(out, "Y_IMAGE"), return NULL,
"%s: Missing column: %s", filename_cat, "Y_IMAGE");
assure( cpl_table_has_column(out, "FWHM_IMAGE"), return NULL,
"%s: Missing column: %s", filename_cat, "FWHM_IMAGE");
assure( cpl_table_has_column(out, "A_IMAGE"), return NULL,
"%s: Missing column: %s", filename_cat, "A_IMAGE");
assure( cpl_table_has_column(out, "B_IMAGE"), return NULL,
"%s: Missing column: %s", filename_cat, "B_IMAGE");
assure( cpl_table_has_column(out, "THETA_IMAGE"), return NULL,
"%s: Missing column: %s", filename_cat, "THETA_IMAGE");
assure( cpl_table_has_column(out, sex_mag), return NULL,
"%s: Missing column: %s", filename_cat, sex_mag);
assure( cpl_table_has_column(out, sex_magerr), return NULL,
"%s: Missing column: %s", filename_cat, sex_magerr);
/* cpl_table_dump_structure(out, stdout); */
if (vignetted) {
cpl_table_add_scalar(out, "X_IMAGE", croplx - 1);
cpl_table_add_scalar(out, "Y_IMAGE", croply - 1);
}
stars = fors_star_list_new();
{
int i;
int bkg_rejected = 0;
int rejected = 0;
int nx = cpl_image_get_size_x(bmaxsigma);
int ny = cpl_image_get_size_y(bmaxsigma);
for (i = 0; i < cpl_table_get_nrow(out); i++) {
fors_star *s = NULL;
unsigned int flags = 0x0;
int x, y, tmp;
double bg_err;
s = fors_star_new_from_table( out,
i,
"X_IMAGE",
"Y_IMAGE",
"FWHM_IMAGE",
"A_IMAGE",
"B_IMAGE",
"THETA_IMAGE",
sex_mag,
sex_magerr,
"CLASS_STAR");
(*s).orientation *= M_PI/180;
(*s).semi_major *= setting->binx;
(*s).semi_minor *= setting->binx;
(*s).fwhm *= setting->binx;
(*s).dmagnitude = sqrt((*s).dmagnitude * (*s).dmagnitude + magsyserr * magsyserr);
flags = cpl_table_get_int( out, "FLAGS", i, NULL);
x = (int)(s->pixel->x + 0.5);
y = (int)(s->pixel->y + 0.5);
if (x >= 1 && x <= nx && y >= 1 && y <= ny)
bg_err = cpl_image_get(bmaxsigma, x, y, &tmp);
else
bg_err = -1.0;
if (fors_extract_check_sex_flag(flags)
&& fors_extract_check_sex_star(s, bmaxsigma)
&& bg_err < level)
{
cpl_msg_debug( cpl_func,
"Source at (%f, %f): fwhm = %f px",
s->pixel->x, s->pixel->y, s->fwhm);
assure( !cpl_error_get_code(), return NULL,
"Could not read SExtractor "
"output table %s",
filename_cat);
fors_star_list_insert(stars, s);
}
else
{
cpl_msg_debug( cpl_func,
"Rejecting source at (%f, %f): "
"flags = 0x%x; fwhm = %f pix; "
"background error = %f; "
"level = %f; "
"background = %f",
s->pixel->x, s->pixel->y,
flags, s->fwhm,
bg_err, level,
cpl_table_get_float(
out, "BACKGROUND", i, NULL));
fors_star_delete(&s);
rejected++;
if (bg_err >= level)
bkg_rejected++;
}
}
cpl_msg_info(cpl_func, "%d sources sextracted, %d rejected",
fors_star_list_size(stars) + rejected,
rejected);
}
if (extracted_sources != NULL) {
*extracted_sources = cpl_table_duplicate(out);
}
cleanup;
return stars;
}
/*----------------------------------------------------------------------------*/
#undef cleanup
#define cleanup
/**
* @brief Extract sources
* @param sky_stats (output) sky statistics
* @param background (output) background
* @param extracted_sources (output) if non-NULL, table of sources
* @return newly allocated list of extracted stars
*
* The star positions are hardcoded!
*
* This method is used only for testing without relying on external
* packages
*/
/*----------------------------------------------------------------------------*/
static fors_star_list *
extract_test( fors_extract_sky_stats *sky_stats,
cpl_image **background,
cpl_table **extracted_sources)
{
assure( sky_stats != NULL, return NULL, NULL );
assure( background != NULL, return NULL, NULL );
sky_stats->mean = 1;
sky_stats->median = 2;
sky_stats->rms = 3;
*background = cpl_image_new(10, 20, CPL_TYPE_FLOAT); /* Zero, wrong size */
fors_star_list *stars = fors_star_list_new();
struct {
double x, y, magnitude, dmagnitude;
}
data[] = {
{100 , 200, -10, 0.01},
{1100, 200, -11, 0.01},
{1 , 5 , -10, 0.01},
{100 , 1200, -12, 0.01},
{1100, 1200, -13, 0.01}
};
int N = sizeof(data) / sizeof(*data);
int i;
double a = 2;
double b = 1;
double fwhm = 1.5;
double orientation = 1.0; /* radians */
for (i = 0; i < N; i++) {
fors_star_list_insert(stars,
fors_star_new(data[i].x,
data[i].y,
fwhm,
a, b, orientation,
data[i].magnitude,
data[i].dmagnitude,
1.0));
}
if (extracted_sources != NULL) {
*extracted_sources = fors_create_sources_table(stars);
assure (!cpl_error_get_code(), return NULL,
"Could not create extracted sources table");
}
return stars;
}
/**@}*/
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