ENH address CR installment 2 (#497)

.gitignore

@@ -52,6 +52,7 @@ examples/ccl_sample_pkemu
 examples/ccl_sample_power
 examples/ccl_sample_run
 examples/ccl_sample_angpow
+examples/*.pdf
 
 # Ignore Python pyc, autogenerated swig files, and build dirs
 *.pyc

CMakeLists.txt

@@ -18,7 +18,7 @@ project(ccl VERSION 0.2.1)
     # Defines list of CCL tests src files
     # ! Add new tests to this list
     set(TEST_SRC tests/ccl_test.c tests/ccl_test_utils.c tests/ccl_test_params.c tests/ccl_test_params_mnu.c
-                 tests/ccl_test_cosmology.c
+	             tests/ccl_test_cosmology.c
     		 tests/ccl_test_distances_class_allz.c tests/ccl_test_distances_cosmomad_hiz.c tests/ccl_test_distances_cosmomad_lowz.c
                  tests/ccl_test_distances_astropy_mnu_lowz.c tests/ccl_test_distances_astropy_mnu_hiz.c
 		 tests/ccl_test_growth_lowz.c tests/ccl_test_growth_hiz.c tests/ccl_test_growth_allz.c

include/ccl_background.h

@@ -14,7 +14,7 @@ typedef enum ccl_species_x_label {
   ccl_species_ur_label=5,
   ccl_species_nu_label=6,
 } ccl_species_x_label;
-  
+
 /**
  * Normalized expansion rate at scale factor a.
  * Returns H(a)/H0 in a given cosmology.
@@ -26,9 +26,6 @@ typedef enum ccl_species_x_label {
  */
 double ccl_h_over_h0(ccl_cosmology * cosmo, double a, int * status);
 
-// Normalized expansion rate at scale factors as given in list a[0..na-1]
-void ccl_h_over_h0s(ccl_cosmology * cosmo, int na, double a[], double output[], int * status);
-
 /**
  * Normalized expansion rate at scale factors as given in list a[0..na-1]
  * Returns H(a)/H0 for an array of scale factors a of length na.
@@ -52,9 +49,6 @@ void ccl_h_over_h0s(ccl_cosmology * cosmo, int na, double a[], double output[],
  */
 double ccl_comoving_radial_distance(ccl_cosmology * cosmo, double a, int* status);
 
-// Comoving radial distances in Mpc to scale factors as given in list a[0..na-1]
-void ccl_comoving_radial_distances(ccl_cosmology * cosmo, int na, double a[], double output[], int* status);
-
 /**
  * Comoving radial distances in Mpc to scale factors as given in list a[0..na-1]
  * @param cosmo Cosmological parameters
@@ -94,9 +88,6 @@ double ccl_sinn(ccl_cosmology *cosmo,double chi, int *status);
  */
 double ccl_comoving_angular_distance(ccl_cosmology * cosmo, double a, int* status);
 
-// Comoving angular distances in Mpc to scale factors as given in list a[0..na-1]
-void ccl_comoving_angular_distances(ccl_cosmology * cosmo, int na, double a[], double output[], int* status);
-
 /**
  * Comoving angular distances in Mpc to scale factors as given in array a[0..na-1]
  * NOTE this quantity is otherwise known as the transverse comoving distance, and is NOT angular diameter
@@ -122,9 +113,6 @@ void ccl_comoving_angular_distances(ccl_cosmology * cosmo, int na, double a[], d
  */
 double ccl_luminosity_distance(ccl_cosmology * cosmo, double a, int * status);
 
-// Comoving luminosity distances in Mpc to scale factors as given in list a[0..na-1]
-void ccl_luminosity_distances(ccl_cosmology * cosmo, int na, double a[], double output[], int * status);
-
 /**
  * Comoving luminosity distances in Mpc to scale factors as given in array a[0..na-1]
  * @param cosmo Cosmological parameters
@@ -172,9 +160,6 @@ void ccl_distance_moduli(ccl_cosmology * cosmo, int na, double a[], double outpu
  */
 double ccl_growth_factor(ccl_cosmology * cosmo, double a, int * status);
 
-// Growth factors at a list of scale factor given in a[0..na-1] normalized to 1 at z=0
-void ccl_growth_factors(ccl_cosmology * cosmo, int na, double a[], double output[], int * status);
-
 /**
  * Growth factors at an array of scale factor given in a[0..na-1], where g(z=0) is normalized to 1
  * @param cosmo Cosmological parameters
@@ -198,9 +183,6 @@ void ccl_growth_factors(ccl_cosmology * cosmo, int na, double a[], double output
  */
 double ccl_growth_factor_unnorm(ccl_cosmology * cosmo, double a, int * status);
 
-// Growth factors at a list of scale factor given in a[0..na-1] normalized to a in matter domination
-void ccl_growth_factors_unnorm(ccl_cosmology * cosmo, int na, double a[], double output[], int * status);
-
 /**
  * Growth factors at a list of scale factor given in a[0..na-1], where g(a) is normalized to a in matter domination
  * @param cosmo Cosmological parameters
@@ -224,9 +206,6 @@ void ccl_growth_factors_unnorm(ccl_cosmology * cosmo, int na, double a[], double
  */
 double ccl_growth_rate(ccl_cosmology * cosmo, double a, int* status);
 
-// Logarithmic rates of d ln g/d lna a at alist of  scale factor a [0..na-1]
-void ccl_growth_rates(ccl_cosmology * cosmo, int na, double a[], double output[], int * status);
-
 /**
  * Logarithmic rates of d ln(g)/d ln(a) at an array of scale factors a[0..na-1]
  * @param cosmo Cosmological parameters
@@ -250,9 +229,6 @@ void ccl_growth_rates(ccl_cosmology * cosmo, int na, double a[], double output[]
  */
 double ccl_scale_factor_of_chi(ccl_cosmology * cosmo, double chi, int * status);
 
-// Scale factors for a given list of comoving distances
-void ccl_scale_factor_of_chis(ccl_cosmology * cosmo, int nchi, double chi[], double output[], int* status);
-
 /**
  * Scale factors for a given array of comoving distances chi[0..nchi-1]
  * @param cosmo Cosmological parameters
@@ -272,9 +248,9 @@ void ccl_scale_factor_of_chis(ccl_cosmology * cosmo, int nchi, double chi[], dou
  * @param a scale factor, normalized to 1 for today
  * @param label species type. Available: 'critical'(0), 'matter'(1), 'dark_energy'(2), 'radiation'(3), 'curvature'(4), 'massless neutrinos'(5), 'massive neutrinos'(6).
  * @param int is_comoving. 0 for physical densities, and nonzero for comoving densities (via a^3 factor).
- * @param status Status flag. 0 if there are no errors, nonzero otherwise. 
+ * @param status Status flag. 0 if there are no errors, nonzero otherwise.
  * For specific cases see documentation for ccl_error.
- * @return rho_x, physical density at scale factor a. 
+ * @return rho_x, physical density at scale factor a.
  */
 double ccl_rho_x(ccl_cosmology * cosmo, double a, ccl_species_x_label label, int is_comoving, int* status);