Deprecated List

Member cpl_fits_get_extension_nb (const char *filename, const char *extname)

Replace this call with cpl_fits_find_extension().

Member cpl_fits_get_nb_extensions (const char *filename)

Replace this call with cpl_fits_count_extensions().

Member cpl_image_filter_linear (const cpl_image *in, const cpl_matrix *ker)

Replace this call with cpl_image_filter() using CPL_FILTER_LINEAR and CPL_BORDER_FILTER.

Member cpl_image_filter_median (const cpl_image *in, const cpl_matrix *ker)

Replace this call with cpl_image_filter_mask() using CPL_FILTER_MEDIAN and CPL_BORDER_FILTER.

Member cpl_image_filter_morpho (const cpl_image *in, const cpl_matrix *ker)

Replace this call with cpl_image_filter() using CPL_FILTER_MORPHO and CPL_BORDER_FILTER.

Member cpl_image_filter_stdev (const cpl_image *in, const cpl_matrix *ker)

Replace this call with cpl_image_filter_mask() using CPL_FILTER_STDEV and CPL_BORDER_FILTER.

Member cpl_image_fit_gaussian (const cpl_image *im, int xpos, int ypos, int size, double *norm, double *xcen, double *ycen, double *sig_x, double *sig_y, double *fwhm_x, double *fwhm_y)

If you need a 2D gaussian fit please use the function cpl_fit_image_gaussian(). Please note that on CPL versions earlier than 5.1.0 this function was wrongly documented: the parameters sig_x and sig_y were defined as "the sigma in x (or y) of the gaussian", while actually they returned the semi-major and semi-minor axes of the gaussian distribution at 1-sigma. PLEASE NOTE THAT IF YOU USED THIS FUNCTION FOR DETERMINING THE SPREAD OF A DISTRIBUTION ALONG THE X DIRECTION, THIS WAS VERY LIKELY OVERESTIMATED (because sig_x was always assigned the semi-major axis of the distribution ignoring the rotation), WHILE THE SPREAD ALONG THE Y DIRECTION WOULD BE UNDERESTIMATED. In addition to that, even with circular distributions this function may lead to an underestimation of sig_x and sig_y (up to 25% underestimation in the case of noiseless data with a box 4 times the sigma, 1% underestimation in the case of noiseless data with a box 7 times the sigma). This latter problem is related to the function cpl_image_iqe().

Member cpl_mask_closing (cpl_mask *in, const cpl_matrix *ker)

Replace this call with cpl_mask_filter() using CPL_FILTER_CLOSING and CPL_BORDER_ZERO.

Member cpl_mask_dilation (cpl_mask *in, const cpl_matrix *ker)

Replace this call with cpl_mask_filter() using CPL_FILTER_DILATION and CPL_BORDER_ZERO.

Member cpl_mask_erosion (cpl_mask *in, const cpl_matrix *ker)

Replace this call with cpl_mask_filter() using CPL_FILTER_EROSION and CPL_BORDER_ZERO.

Member cpl_mask_opening (cpl_mask *in, const cpl_matrix *ker)

Replace this call with cpl_mask_filter() using CPL_FILTER_OPENING and CPL_BORDER_ZERO.

Member cpl_msg_progress (const char *component, int i, int iter, const char *format,...)

Use standard calls such as cpl_msg_info() instead.

Member cpl_polynomial_fit_1d_create (const cpl_vector *x_pos, const cpl_vector *values, int degree, double *mse)

Replace this call with cpl_polynomial_fit() and optionally cpl_vector_fill_polynomial_fit_residual().

Member cpl_polynomial_fit_2d_create (cpl_bivector *xy_pos, cpl_vector *values, int degree, double *mse)

Replace this call with cpl_polynomial_fit() and optionally cpl_vector_fill_polynomial_fit_residual().

Member CPL_RECIPE_DEFINE (RECIPE_NAME, RECIPE_VERSION, RECIPE_FILL_PARAMS,RECIPE_AUTHOR, RECIPE_AUTHOR_EMAIL, RECIPE_YEAR,RECIPE_SYNOPSIS, RECIPE_DESCRIPTION)

Use cpl_recipe_define()

Member cpl_vector_convolve_symmetric (cpl_vector *smoothed, const cpl_vector *conv_kernel)

Unstable API, may change or disappear. Do not use in new code!

Member cpl_vector_new_lss_kernel (double slitw, double fwhm)

Unstable API, may change or disappear. Do not use in new code!