MAINT: Delete classy function (#560)

skypyproject · Jul 1, 2022 · 9733d25 · 9733d25
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diff --git a/docs/power_spectrum/index.rst b/docs/power_spectrum/index.rst
@@ -5,7 +5,7 @@ This module contains methods to model the matter power spectrum.
 
 SkyPy provides wrappers to a number of external codes for calculating the
 matter power spectrum, including `~skypy.power_spectrum.CAMB` and
-`~skypy.power_spectrum.classy`. Here we demonstrate calculating the linear
+`~skypy.power_spectrum.CLASSY`. Here we demonstrate calculating the linear
 matter power spectrum using `~skypy.power_spectrum.eisenstein_hu` and the
 non-linear corrections using `~skypy.power_spectrum.halofit_smith`:
 

diff --git a/skypy/power_spectrum/__init__.py b/skypy/power_spectrum/__init__.py
@@ -9,7 +9,7 @@
    :toctree: ../api/
 
    CAMB
-   classy
+   CLASSY
    eisenstein_hu
    transfer_no_wiggles
    transfer_with_wiggles

diff --git a/skypy/power_spectrum/_classy.py b/skypy/power_spectrum/_classy.py
@@ -3,80 +3,9 @@
 
 __all__ = [
     'CLASSY',
-    'classy',
 ]
 
 
-def classy(wavenumber, redshift, cosmology, **kwargs):
-    """ Return the CLASS computation of the linear matter power spectrum, on a
-    two dimensional grid of wavenumber and redshift.
-
-    Additional CLASS parameters can be passed via keyword arguments.
-
-    Parameters
-    ----------
-    wavenumber : (nk,) array_like
-        Array of wavenumbers in units of Mpc-1 at which to
-        evaluate the linear matter power spectrum.
-    redshift : (nz,) array_like
-        Array of redshifts at which to evaluate the linear matter power
-        spectrum.
-    cosmology : astropy.cosmology.Cosmology
-        Cosmology object providing omega_matter, omega_baryon, Hubble
-        parameter and CMB temperature in the present day
-
-    Returns
-    -------
-    power_spectrum : (nz, nk) array_like
-        Array of values for the linear matter power spectrum in Mpc3
-        evaluated at the input wavenumbers for the given primordial power
-        spectrum parameters, cosmology. For nz redshifts and nk wavenumbers
-        the returned array will have shape (nz, nk).
-
-    References
-    ----------
-    doi : 10.1088/1475-7516/2011/07/034
-    arXiv: 1104.2932, 1104.2933
-
-    """
-    try:
-        from classy import Class
-    except ImportError:
-        raise Exception("classy is required to use skypy.linear.classy")
-
-    h2 = cosmology.h * cosmology.h
-
-    params = {
-        'output': 'mPk',
-        'P_k_max_1/Mpc':  np.max(wavenumber),
-        'z_pk': ', '.join(str(z) for z in np.atleast_1d(redshift)),
-        'H0':        cosmology.H0.value,
-        'omega_b':   cosmology.Ob0 * h2,
-        'omega_cdm': cosmology.Odm0 * h2,
-        'T_cmb':     cosmology.Tcmb0.value,
-        'N_eff':     cosmology.Neff,
-    }
-
-    params.update(kwargs)
-
-    classy_obj = Class()
-    classy_obj.set(params)
-    classy_obj.compute()
-
-    z = np.expand_dims(redshift, (-1,)*np.ndim(wavenumber))
-    k = np.expand_dims(wavenumber, (0,)*np.ndim(redshift))
-    z, k = np.broadcast_arrays(z, k)
-    pzk = np.empty(z.shape)
-
-    for i in np.ndindex(*pzk.shape):
-        pzk[i] = classy_obj.pk_lin(k[i], z[i])
-
-    if pzk.ndim == 0:
-        pzk = pzk.item()
-
-    return pzk
-
-
 class CLASSY(TabulatedPowerSpectrum):
 
     def __init__(self, kmax, redshift, cosmology, **kwargs):