# Docstrings for generated ufuncs
#
# The syntax is designed to look like the function add_newdoc is being
# called from numpy.lib, but in this file add_newdoc puts the
# docstrings in a dictionary. This dictionary is used in
# generate_ufuncs.py to generate the docstrings for the ufuncs in
# scipy.special at the C level when the ufuncs are created at compile
# time.

from __future__ import division, print_function, absolute_import

docdict = {}


def get(name):
    return docdict.get(name)


def add_newdoc(place, name, doc):
    docdict['.'.join((place, name))] = doc

add_newdoc("scipy.special", "sph_harm",
    r"""
    sph_harm(m, n, theta, phi)

    Compute spherical harmonics.

    .. math:: Y^m_n(\theta,\phi) = \sqrt{\frac{2n+1}{4\pi}\frac{(n-m)!}{(n+m)!}} e^{i m \theta} P^m_n(\cos(\phi))

    Parameters
    ----------
    m : int
       ``|m| <= n``; the order of the harmonic.
    n : int
       where `n` >= 0; the degree of the harmonic.  This is often called
       ``l`` (lower case L) in descriptions of spherical harmonics.
    theta : float
       [0, 2*pi]; the azimuthal (longitudinal) coordinate.
    phi : float
       [0, pi]; the polar (colatitudinal) coordinate.

    Returns
    -------
    y_mn : complex float
       The harmonic :math:`Y^m_n` sampled at `theta` and `phi`

    Notes
    -----
    There are different conventions for the meaning of input arguments
    `theta` and `phi`.  We take `theta` to be the azimuthal angle and
    `phi` to be the polar angle.  It is common to see the opposite
    convention - that is `theta` as the polar angle and `phi` as the
    azimuthal angle.

    References
    ----------
    .. [1] Digital Library of Mathematical Functions, 14.30. http://dlmf.nist.gov/14.30
    """)

add_newdoc("scipy.special", "_ellip_harm",
    """
    Internal function, use `ellip_harm` instead.
    """)

add_newdoc("scipy.special", "_ellip_norm",
    """
    Internal function, use `ellip_norm` instead.
    """)

add_newdoc("scipy.special", "_lambertw",
    """
    Internal function, use `lambertw` instead.
    """)

add_newdoc("scipy.special", "airy",
    """
    airy(z)

    Airy functions and their derivatives.

    Parameters
    ----------
    z : float or complex
        Argument.

    Returns
    -------
    Ai, Aip, Bi, Bip
        Airy functions Ai and Bi, and their derivatives Aip and Bip

    Notes
    -----
    The Airy functions Ai and Bi are two independent solutions of y''(x) = x y.

    """)

add_newdoc("scipy.special", "airye",
    """
    airye(z)

    Exponentially scaled Airy functions and their derivatives.

    Scaling::

        eAi  = Ai  * exp(2.0/3.0*z*sqrt(z))
        eAip = Aip * exp(2.0/3.0*z*sqrt(z))
        eBi  = Bi  * exp(-abs((2.0/3.0*z*sqrt(z)).real))
        eBip = Bip * exp(-abs((2.0/3.0*z*sqrt(z)).real))

    Parameters
    ----------
    z : float or complex
        Argument.

    Returns
    -------
    eAi, eAip, eBi, eBip
        Airy functions Ai and Bi, and their derivatives Aip and Bip

    """)

add_newdoc("scipy.special", "bdtr",
    """
    bdtr(k, n, p)

    Binomial distribution cumulative distribution function.

    Sum of the terms 0 through k of the Binomial probability density.

    ::

        y = sum(nCj p**j (1-p)**(n-j),j=0..k)

    Parameters
    ----------
    k, n : int
        Terms to include
    p : float
        Probability

    Returns
    -------
    y : float
        Sum of terms

    """)

add_newdoc("scipy.special", "bdtrc",
    """
    bdtrc(k, n, p)

    Binomial distribution survival function.

    Sum of the terms k+1 through n of the Binomial probability density

    ::

        y = sum(nCj p**j (1-p)**(n-j), j=k+1..n)

    Parameters
    ----------
    k, n : int
        Terms to include
    p : float
        Probability

    Returns
    -------
    y : float
        Sum of terms

    """)

add_newdoc("scipy.special", "bdtri",
    """
    bdtri(k, n, y)

    Inverse function to bdtr vs. p

    Finds probability `p` such that for the cumulative binomial
    probability ``bdtr(k, n, p) == y``.
    """)

add_newdoc("scipy.special", "bdtrik",
    """
    bdtrik(y, n, p)

    Inverse function to bdtr vs k
    """)

add_newdoc("scipy.special", "bdtrin",
    """
    bdtrin(k, y, p)

    Inverse function to bdtr vs n
    """)

add_newdoc("scipy.special", "binom",
    """
    binom(n, k)

    Binomial coefficient
    """)

add_newdoc("scipy.special", "btdtria",
    """
    btdtria(p, b, x)

    Inverse of btdtr vs a

    """)

add_newdoc("scipy.special", "btdtrib",
    """
    btdtria(a, p, x)

    Inverse of btdtr vs b

    """)

add_newdoc("scipy.special", "bei",
    """
    bei(x)

    Kelvin function bei
    """)

add_newdoc("scipy.special", "beip",
    """
    beip(x)

    Derivative of the Kelvin function bei
    """)

add_newdoc("scipy.special", "ber",
    """
    ber(x)

    Kelvin function ber.
    """)

add_newdoc("scipy.special", "berp",
    """
    berp(x)

    Derivative of the Kelvin function ber
    """)

add_newdoc("scipy.special", "besselpoly",
    r"""
    besselpoly(a, lmb, nu)

    Weighed integral of a Bessel function.

    .. math::

       \int_0^1 x^\lambda J_v(\nu, 2 a x) \, dx

    where :math:`J_v` is a Bessel function and :math:`\lambda=lmb`,
    :math:`\nu=nu`.

    """)

add_newdoc("scipy.special", "beta",
    """
    beta(a, b)

    Beta function.

    ::

        beta(a,b) =  gamma(a) * gamma(b) / gamma(a+b)
    """)

add_newdoc("scipy.special", "betainc",
    """
    betainc(a, b, x)

    Incomplete beta integral.

    Compute the incomplete beta integral of the arguments, evaluated
    from zero to x::

        gamma(a+b) / (gamma(a)*gamma(b)) * integral(t**(a-1) (1-t)**(b-1), t=0..x).

    Notes
    -----
    The incomplete beta is also sometimes defined without the terms
    in gamma, in which case the above definition is the so-called regularized
    incomplete beta. Under this definition, you can get the incomplete beta by
    multiplying the result of the scipy function by beta(a, b).

    """)

add_newdoc("scipy.special", "betaincinv",
    """
    betaincinv(a, b, y)

    Inverse function to beta integral.

    Compute x such that betainc(a,b,x) = y.
    """)

add_newdoc("scipy.special", "betaln",
    """
    betaln(a, b)

    Natural logarithm of absolute value of beta function.

    Computes ``ln(abs(beta(x)))``.
    """)

add_newdoc("scipy.special", "boxcox",
    """
    boxcox(x, lmbda)

    Compute the Box-Cox transformation.

    The Box-Cox transformation is::

        y = (x**lmbda - 1) / lmbda  if lmbda != 0
            log(x)                  if lmbda == 0

    Returns `nan` if ``x < 0``.
    Returns `-inf` if ``x == 0`` and ``lmbda < 0``.

    Parameters
    ----------
    x : array_like
        Data to be transformed.
    lmbda : array_like
        Power parameter of the Box-Cox transform.

    Returns
    -------
    y : array
        Transformed data.

    Notes
    -----

    .. versionadded:: 0.14.0

    Examples
    --------
    >>> boxcox([1, 4, 10], 2.5)
    array([   0.        ,   12.4       ,  126.09110641])
    >>> boxcox(2, [0, 1, 2])
    array([ 0.69314718,  1.        ,  1.5       ])
    """)

add_newdoc("scipy.special", "boxcox1p",
    """
    boxcox1p(x, lmbda)

    Compute the Box-Cox transformation of 1 + `x`.

    The Box-Cox transformation computed by `boxcox1p` is::

        y = ((1+x)**lmbda - 1) / lmbda  if lmbda != 0
            log(1+x)                    if lmbda == 0

    Returns `nan` if ``x < -1``.
    Returns `-inf` if ``x == -1`` and ``lmbda < 0``.

    Parameters
    ----------
    x : array_like
        Data to be transformed.
    lmbda : array_like
        Power parameter of the Box-Cox transform.

    Returns
    -------
    y : array
        Transformed data.

    Notes
    -----

    .. versionadded:: 0.14.0

    Examples
    --------
    >>> boxcox1p(1e-4, [0, 0.5, 1])
    array([  9.99950003e-05,   9.99975001e-05,   1.00000000e-04])
    >>> boxcox1p([0.01, 0.1], 0.25)
    array([ 0.00996272,  0.09645476])
    """)

add_newdoc("scipy.special", "inv_boxcox",
    """
    inv_boxcox(y, lmbda)

    Compute the inverse of the Box-Cox transformation.

    Find ``x`` such that::

        y = (x**lmbda - 1) / lmbda  if lmbda != 0
            log(x)                  if lmbda == 0

    Parameters
    ----------
    y : array_like
        Data to be transformed.
    lmbda : array_like
        Power parameter of the Box-Cox transform.

    Returns
    -------
    x : array
        Transformed data.

    Notes
    -----

    .. versionadded:: 0.16.0

    Examples
    --------
    >>> y = boxcox([1, 4, 10], 2.5)
    >>> inv_boxcox(y, 2.5)
    array([1., 4., 10.])
    """)

add_newdoc("scipy.special", "inv_boxcox1p",
    """
    inv_boxcox1p(y, lmbda)

    Compute the inverse of the Box-Cox transformation.

    Find ``x`` such that::

        y = ((1+x)**lmbda - 1) / lmbda  if lmbda != 0
            log(1+x)                    if lmbda == 0

    Parameters
    ----------
    y : array_like
        Data to be transformed.
    lmbda : array_like
        Power parameter of the Box-Cox transform.

    Returns
    -------
    x : array
        Transformed data.

    Notes
    -----

    .. versionadded:: 0.16.0

    Examples
    --------
    >>> y = boxcox1p([1, 4, 10], 2.5)
    >>> inv_boxcox1p(y, 2.5)
    array([1., 4., 10.])
    """)

add_newdoc("scipy.special", "btdtr",
    """
    btdtr(a,b,x)

    Cumulative beta distribution.

    Returns the area from zero to x under the beta density function::

        gamma(a+b)/(gamma(a)*gamma(b)))*integral(t**(a-1) (1-t)**(b-1), t=0..x)

    See Also
    --------
    betainc
    """)

add_newdoc("scipy.special", "btdtri",
    """
    btdtri(a,b,p)

    p-th quantile of the beta distribution.

    This is effectively the inverse of btdtr returning the value of x for which
    ``btdtr(a,b,x) = p``

    See Also
    --------
    betaincinv
    """)

add_newdoc("scipy.special", "cbrt",
    """
    cbrt(x)

    Cube root of x
    """)

add_newdoc("scipy.special", "chdtr",
    """
    chdtr(v, x)

    Chi square cumulative distribution function

    Returns the area under the left hand tail (from 0 to x) of the Chi
    square probability density function with v degrees of freedom::

        1/(2**(v/2) * gamma(v/2)) * integral(t**(v/2-1) * exp(-t/2), t=0..x)
    """)

add_newdoc("scipy.special", "chdtrc",
    """
    chdtrc(v,x)

    Chi square survival function

    Returns the area under the right hand tail (from x to
    infinity) of the Chi square probability density function with v
    degrees of freedom::

        1/(2**(v/2) * gamma(v/2)) * integral(t**(v/2-1) * exp(-t/2), t=x..inf)
    """)

add_newdoc("scipy.special", "chdtri",
    """
    chdtri(v,p)

    Inverse to chdtrc

    Returns the argument x such that ``chdtrc(v,x) == p``.
    """)

add_newdoc("scipy.special", "chdtriv",
    """
    chdtri(p, x)

    Inverse to chdtr vs v

    Returns the argument v such that ``chdtr(v, x) == p``.
    """)

add_newdoc("scipy.special", "chndtr",
    """
    chndtr(x, df, nc)

    Non-central chi square cumulative distribution function

    """)

add_newdoc("scipy.special", "chndtrix",
    """
    chndtrix(p, df, nc)

    Inverse to chndtr vs x
    """)

add_newdoc("scipy.special", "chndtridf",
    """
    chndtridf(x, p, nc)

    Inverse to chndtr vs df
    """)

add_newdoc("scipy.special", "chndtrinc",
    """
    chndtrinc(x, df, p)

    Inverse to chndtr vs nc
    """)

add_newdoc("scipy.special", "cosdg",
    """
    cosdg(x)

    Cosine of the angle x given in degrees.
    """)

add_newdoc("scipy.special", "cosm1",
    """
    cosm1(x)

    cos(x) - 1 for use when x is near zero.
    """)

add_newdoc("scipy.special", "cotdg",
    """
    cotdg(x)

    Cotangent of the angle x given in degrees.
    """)

add_newdoc("scipy.special", "dawsn",
    """
    dawsn(x)

    Dawson's integral.

    Computes::

        exp(-x**2) * integral(exp(t**2),t=0..x).

    References
    ----------
    .. [1] Steven G. Johnson, Faddeeva W function implementation.
       http://ab-initio.mit.edu/Faddeeva
    """)

add_newdoc("scipy.special", "ellipe",
    """
    ellipe(m)

    Complete elliptic integral of the second kind

    This function is defined as

    .. math:: E(m) = \\int_0^{\\pi/2} [1 - m \\sin(t)^2]^{1/2} dt

    Parameters
    ----------
    m : array_like
        Defines the parameter of the elliptic integral.

    Returns
    -------
    E : ndarray
        Value of the elliptic integral.

    See Also
    --------
    ellipkm1 : Complete elliptic integral of the first kind, near  m = 1
    ellipk : Complete elliptic integral of the first kind
    ellipkinc : Incomplete elliptic integral of the first kind
    ellipeinc : Incomplete elliptic integral of the second kind
    """)

add_newdoc("scipy.special", "ellipeinc",
    """
    ellipeinc(phi, m)

    Incomplete elliptic integral of the second kind

    This function is defined as

    .. math:: E(\\phi, m) = \\int_0^{\\phi} [1 - m \\sin(t)^2]^{1/2} dt

    Parameters
    ----------
    phi : array_like
        amplitude of the elliptic integral.

    m : array_like
        parameter of the elliptic integral.

    Returns
    -------
    E : ndarray
        Value of the elliptic integral.

    See Also
    --------
    ellipkm1 : Complete elliptic integral of the first kind, near m = 1
    ellipk : Complete elliptic integral of the first kind
    ellipkinc : Incomplete elliptic integral of the first kind
    ellipe : Complete elliptic integral of the second kind
    """)

add_newdoc("scipy.special", "ellipj",
    """
    ellipj(u, m)

    Jacobian elliptic functions

    Calculates the Jacobian elliptic functions of parameter m between
    0 and 1, and real u.

    Parameters
    ----------
    m, u
        Parameters

    Returns
    -------
    sn, cn, dn, ph
        The returned functions::

            sn(u|m), cn(u|m), dn(u|m)

        The value ``ph`` is such that if ``u = ellik(ph, m)``,
        then ``sn(u|m) = sin(ph)`` and ``cn(u|m) = cos(ph)``.

    """)

add_newdoc("scipy.special", "ellipkm1",
    """
    ellipkm1(p)

    Complete elliptic integral of the first kind around m = 1

    This function is defined as

    .. math:: K(p) = \\int_0^{\\pi/2} [1 - m \\sin(t)^2]^{-1/2} dt

    where `m = 1 - p`.

    Parameters
    ----------
    p : array_like
        Defines the parameter of the elliptic integral as m = 1 - p.

    Returns
    -------
    K : ndarray
        Value of the elliptic integral.

    See Also
    --------
    ellipk : Complete elliptic integral of the first kind
    ellipkinc : Incomplete elliptic integral of the first kind
    ellipe : Complete elliptic integral of the second kind
    ellipeinc : Incomplete elliptic integral of the second kind
    """)

add_newdoc("scipy.special", "ellipkinc",
    """
    ellipkinc(phi, m)

    Incomplete elliptic integral of the first kind

    This function is defined as

    .. math:: K(\\phi, m) = \\int_0^{\\phi} [1 - m \\sin(t)^2]^{-1/2} dt

    Parameters
    ----------
    phi : array_like
        amplitude of the elliptic integral

    m : array_like
        parameter of the elliptic integral

    Returns
    -------
    K : ndarray
        Value of the elliptic integral

    Notes
    -----
    This function is also called ``F(phi, m)``.

    See Also
    --------
    ellipkm1 : Complete elliptic integral of the first kind, near  m = 1
    ellipk : Complete elliptic integral of the first kind
    ellipe : Complete elliptic integral of the second kind
    ellipeinc : Incomplete elliptic integral of the second kind

    """)

add_newdoc("scipy.special", "entr",
    r"""
    entr(x)

    Elementwise function for computing entropy.

    .. math:: \text{entr}(x) = \begin{cases} - x \log(x) & x > 0  \\ 0 & x = 0 \\ -\infty & \text{otherwise} \end{cases}

    Parameters
    ----------
    x : ndarray
        Input array.

    Returns
    -------
    res : ndarray
        The value of the elementwise entropy function at the given points x.

    See Also
    --------
    kl_div, rel_entr

    Notes
    -----
    This function is concave.

    .. versionadded:: 0.14.0

    """)

add_newdoc("scipy.special", "erf",
    """
    erf(z)

    Returns the error function of complex argument.

    It is defined as ``2/sqrt(pi)*integral(exp(-t**2), t=0..z)``.

    Parameters
    ----------
    x : ndarray
        Input array.

    Returns
    -------
    res : ndarray
        The values of the error function at the given points x.

    See Also
    --------
    erfc, erfinv, erfcinv

    Notes
    -----
    The cumulative of the unit normal distribution is given by
    ``Phi(z) = 1/2[1 + erf(z/sqrt(2))]``.

    References
    ----------
    .. [1] http://en.wikipedia.org/wiki/Error_function
    .. [2] Milton Abramowitz and Irene A. Stegun, eds.
        Handbook of Mathematical Functions with Formulas,
        Graphs, and Mathematical Tables. New York: Dover,
        1972. http://www.math.sfu.ca/~cbm/aands/page_297.htm
    .. [3] Steven G. Johnson, Faddeeva W function implementation.
       http://ab-initio.mit.edu/Faddeeva

    """)

add_newdoc("scipy.special", "erfc",
    """
    erfc(x)

    Complementary error function, 1 - erf(x).

    References
    ----------
    .. [1] Steven G. Johnson, Faddeeva W function implementation.
       http://ab-initio.mit.edu/Faddeeva

    """)

add_newdoc("scipy.special", "erfi",
    """
    erfi(z)

    Imaginary error function, -i erf(i z).

    Notes
    -----

    .. versionadded:: 0.12.0

    References
    ----------
    .. [1] Steven G. Johnson, Faddeeva W function implementation.
       http://ab-initio.mit.edu/Faddeeva

    """)

add_newdoc("scipy.special", "erfcx",
    """
    erfcx(x)

    Scaled complementary error function, exp(x^2) erfc(x).

    Notes
    -----

    .. versionadded:: 0.12.0

    References
    ----------
    .. [1] Steven G. Johnson, Faddeeva W function implementation.
       http://ab-initio.mit.edu/Faddeeva

    """)

add_newdoc("scipy.special", "eval_jacobi",
    """
    eval_jacobi(n, alpha, beta, x, out=None)

    Evaluate Jacobi polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_sh_jacobi",
    """
    eval_sh_jacobi(n, p, q, x, out=None)

    Evaluate shifted Jacobi polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_gegenbauer",
    """
    eval_gegenbauer(n, alpha, x, out=None)

    Evaluate Gegenbauer polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_chebyt",
    """
    eval_chebyt(n, x, out=None)

    Evaluate Chebyshev T polynomial at a point.

    This routine is numerically stable for `x` in ``[-1, 1]`` at least
    up to order ``10000``.
    """)

add_newdoc("scipy.special", "eval_chebyu",
    """
    eval_chebyu(n, x, out=None)

    Evaluate Chebyshev U polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_chebys",
    """
    eval_chebys(n, x, out=None)

    Evaluate Chebyshev S polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_chebyc",
    """
    eval_chebyc(n, x, out=None)

    Evaluate Chebyshev C polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_sh_chebyt",
    """
    eval_sh_chebyt(n, x, out=None)

    Evaluate shifted Chebyshev T polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_sh_chebyu",
    """
    eval_sh_chebyu(n, x, out=None)

    Evaluate shifted Chebyshev U polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_legendre",
    """
    eval_legendre(n, x, out=None)

    Evaluate Legendre polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_sh_legendre",
    """
    eval_sh_legendre(n, x, out=None)

    Evaluate shifted Legendre polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_genlaguerre",
    """
    eval_genlaguerre(n, alpha, x, out=None)

    Evaluate generalized Laguerre polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_laguerre",
     """
    eval_laguerre(n, x, out=None)

    Evaluate Laguerre polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_hermite",
    """
    eval_hermite(n, x, out=None)

    Evaluate Hermite polynomial at a point.
    """)

add_newdoc("scipy.special", "eval_hermitenorm",
    """
    eval_hermitenorm(n, x, out=None)

    Evaluate normalized Hermite polynomial at a point.
    """)

add_newdoc("scipy.special", "exp1",
    """
    exp1(z)

    Exponential integral E_1 of complex argument z

    ::

        integral(exp(-z*t)/t,t=1..inf).
    """)

add_newdoc("scipy.special", "exp10",
    """
    exp10(x)

    10**x
    """)

add_newdoc("scipy.special", "exp2",
    """
    exp2(x)

    2**x
    """)

add_newdoc("scipy.special", "expi",
    """
    expi(x)

    Exponential integral Ei

    Defined as::

        integral(exp(t)/t,t=-inf..x)

    See `expn` for a different exponential integral.
    """)

add_newdoc('scipy.special', 'expit',
    """
    expit(x)

    Expit ufunc for ndarrays.

    The expit function, also known as the logistic function, is defined as
    expit(x) = 1/(1+exp(-x)). It is the inverse of the logit function.

    Parameters
    ----------
    x : ndarray
        The ndarray to apply expit to element-wise.

    Returns
    -------
    out : ndarray
        An ndarray of the same shape as x. Its entries
        are expit of the corresponding entry of x.

    Notes
    -----
    As a ufunc expit takes a number of optional
    keyword arguments. For more information
    see `ufuncs <http://docs.scipy.org/doc/numpy/reference/ufuncs.html>`_

    .. versionadded:: 0.10.0

    """)

add_newdoc("scipy.special", "expm1",
    """
    expm1(x)

    exp(x) - 1 for use when x is near zero.
    """)

add_newdoc("scipy.special", "expn",
    """
    expn(n, x)

    Exponential integral E_n

    Returns the exponential integral for integer n and non-negative x and n::

        integral(exp(-x*t) / t**n, t=1..inf).
    """)

add_newdoc("scipy.special", "fdtr",
    """
    fdtr(dfn, dfd, x)

    F cumulative distribution function

    Returns the area from zero to x under the F density function (also
    known as Snedcor's density or the variance ratio density).  This
    is the density of X = (unum/dfn)/(uden/dfd), where unum and uden
    are random variables having Chi square distributions with dfn and
    dfd degrees of freedom, respectively.
    """)

add_newdoc("scipy.special", "fdtrc",
    """
    fdtrc(dfn, dfd, x)

    F survival function

    Returns the complemented F distribution function.
    """)

add_newdoc("scipy.special", "fdtri",
    """
    fdtri(dfn, dfd, p)

    Inverse to fdtr vs x

    Finds the F density argument x such that ``fdtr(dfn, dfd, x) == p``.
    """)

add_newdoc("scipy.special", "fdtridfd",
    """
    fdtridfd(dfn, p, x)

    Inverse to fdtr vs dfd

    Finds the F density argument dfd such that ``fdtr(dfn,dfd,x) == p``.
    """)

add_newdoc("scipy.special", "fdtridfn",
    """
    fdtridfn(p, dfd, x)

    Inverse to fdtr vs dfn

    finds the F density argument dfn such that ``fdtr(dfn,dfd,x) == p``.
    """)

add_newdoc("scipy.special", "fresnel",
    """
    fresnel(z)

    Fresnel sin and cos integrals

    Defined as::

        ssa = integral(sin(pi/2 * t**2),t=0..z)
        csa = integral(cos(pi/2 * t**2),t=0..z)

    Parameters
    ----------
    z : float or complex array_like
        Argument

    Returns
    -------
    ssa, csa
        Fresnel sin and cos integral values

    """)

add_newdoc("scipy.special", "gamma",
    """
    gamma(z)

    Gamma function

    The gamma function is often referred to as the generalized
    factorial since ``z*gamma(z) = gamma(z+1)`` and ``gamma(n+1) =
    n!`` for natural number *n*.
    """)

add_newdoc("scipy.special", "gammainc",
    """
    gammainc(a, x)

    Incomplete gamma function

    Defined as::

        1 / gamma(a) * integral(exp(-t) * t**(a-1), t=0..x)

    `a` must be positive and `x` must be >= 0.
    """)

add_newdoc("scipy.special", "gammaincc",
    """
    gammaincc(a,x)

    Complemented incomplete gamma integral

    Defined as::

        1 / gamma(a) * integral(exp(-t) * t**(a-1), t=x..inf) = 1 - gammainc(a,x)

    `a` must be positive and `x` must be >= 0.
    """)

add_newdoc("scipy.special", "gammainccinv",
    """
    gammainccinv(a,y)

    Inverse to gammaincc

    Returns `x` such that ``gammaincc(a,x) == y``.
    """)

add_newdoc("scipy.special", "gammaincinv",
    """
    gammaincinv(a, y)

    Inverse to gammainc

    Returns `x` such that ``gammainc(a, x) = y``.
    """)

add_newdoc("scipy.special", "gammaln",
    """
    gammaln(z)

    Logarithm of absolute value of gamma function

    Defined as::

        ln(abs(gamma(z)))

    See Also
    --------
    gammasgn
    """)

add_newdoc("scipy.special", "gammasgn",
    """
    gammasgn(x)

    Sign of the gamma function.

    See Also
    --------
    gammaln
    """)

add_newdoc("scipy.special", "gdtr",
    """
    gdtr(a,b,x)

    Gamma distribution cumulative density function.

    Returns the integral from zero to x of the gamma probability
    density function::

        a**b / gamma(b) * integral(t**(b-1) exp(-at),t=0..x).

    The arguments a and b are used differently here than in other
    definitions.
    """)

add_newdoc("scipy.special", "gdtrc",
    """
    gdtrc(a,b,x)

    Gamma distribution survival function.

    Integral from x to infinity of the gamma probability density
    function.

    See Also
    --------
    gdtr, gdtri
    """)

add_newdoc("scipy.special", "gdtria",
    """
    gdtria(p, b, x, out=None)

    Inverse of gdtr vs a.

    Returns the inverse with respect to the parameter `a` of ``p =
    gdtr(a, b, x)``, the cumulative distribution function of the gamma
    distribution.

    Parameters
    ----------
    p : array_like
        Probability values.
    b : array_like
        `b` parameter values of `gdtr(a, b, x)`.  `b` is the "shape" parameter
        of the gamma distribution.
    x : array_like
        Nonnegative real values, from the domain of the gamma distribution.
    out : ndarray, optional
        If a fourth argument is given, it must be a numpy.ndarray whose size
        matches the broadcast result of `a`, `b` and `x`.  `out` is then the
        array returned by the function.

    Returns
    -------
    a : ndarray
        Values of the `a` parameter such that `p = gdtr(a, b, x)`.  `1/a`
        is the "scale" parameter of the gamma distribution.

    See Also
    --------
    gdtr : CDF of the gamma distribution.
    gdtrib : Inverse with respect to `b` of `gdtr(a, b, x)`.
    gdtrix : Inverse with respect to `x` of `gdtr(a, b, x)`.

    Examples
    --------
    First evaluate `gdtr`.

    >>> p = gdtr(1.2, 3.4, 5.6)
    >>> print(p)
    0.94378087442

    Verify the inverse.

    >>> gdtria(p, 3.4, 5.6)
    1.2
    """)

add_newdoc("scipy.special", "gdtrib",
    """
    gdtrib(a, p, x, out=None)

    Inverse of gdtr vs b.

    Returns the inverse with respect to the parameter `b` of ``p =
    gdtr(a, b, x)``, the cumulative distribution function of the gamma
    distribution.

    Parameters
    ----------
    a : array_like
        `a` parameter values of `gdtr(a, b, x)`. `1/a` is the "scale"
        parameter of the gamma distribution.
    p : array_like
        Probability values.
    x : array_like
        Nonnegative real values, from the domain of the gamma distribution.
    out : ndarray, optional
        If a fourth argument is given, it must be a numpy.ndarray whose size
        matches the broadcast result of `a`, `b` and `x`.  `out` is then the
        array returned by the function.

    Returns
    -------
    b : ndarray
        Values of the `b` parameter such that `p = gdtr(a, b, x)`.  `b` is
        the "shape" parameter of the gamma distribution.

    See Also
    --------
    gdtr : CDF of the gamma distribution.
    gdtria : Inverse with respect to `a` of `gdtr(a, b, x)`.
    gdtrix : Inverse with respect to `x` of `gdtr(a, b, x)`.

    Examples
    --------
    First evaluate `gdtr`.

    >>> p = gdtr(1.2, 3.4, 5.6)
    >>> print(p)
    0.94378087442

    Verify the inverse.

    >>> gdtrib(1.2, p, 5.6)
    3.3999999999723882
    """)

add_newdoc("scipy.special", "gdtrix",
    """
    gdtrix(a, b, p, out=None)

    Inverse of gdtr vs x.

    Returns the inverse with respect to the parameter `x` of ``p =
    gdtr(a, b, x)``, the cumulative distribution function of the gamma
    distribution. This is also known as the p'th quantile of the
    distribution.

    Parameters
    ----------
    a : array_like
        `a` parameter values of `gdtr(a, b, x)`.  `1/a` is the "scale"
        parameter of the gamma distribution.
    b : array_like
        `b` parameter values of `gdtr(a, b, x)`.  `b` is the "shape" parameter
        of the gamma distribution.
    p : array_like
        Probability values.
    out : ndarray, optional
        If a fourth argument is given, it must be a numpy.ndarray whose size
        matches the broadcast result of `a`, `b` and `x`.  `out` is then the
        array returned by the function.

    Returns
    -------
    x : ndarray
        Values of the `x` parameter such that `p = gdtr(a, b, x)`.

    See Also
    --------
    gdtr : CDF of the gamma distribution.
    gdtria : Inverse with respect to `a` of `gdtr(a, b, x)`.
    gdtrib : Inverse with respect to `b` of `gdtr(a, b, x)`.

    Examples
    --------
    First evaluate `gdtr`.

    >>> p = gdtr(1.2, 3.4, 5.6)
    >>> print(p)
    0.94378087442

    Verify the inverse.

    >>> gdtrix(1.2, 3.4, p)
    5.5999999999999996
    """)

add_newdoc("scipy.special", "hankel1",
    """
    hankel1(v, z)

    Hankel function of the first kind

    Parameters
    ----------
    v : float
        Order
    z : float or complex
        Argument

    """)

add_newdoc("scipy.special", "hankel1e",
    """
    hankel1e(v, z)

    Exponentially scaled Hankel function of the first kind

    Defined as::

        hankel1e(v,z) = hankel1(v,z) * exp(-1j * z)

    Parameters
    ----------
    v : float
        Order
    z : complex
        Argument
    """)

add_newdoc("scipy.special", "hankel2",
    """
    hankel2(v, z)

    Hankel function of the second kind

    Parameters
    ----------
    v : float
        Order
    z : complex
        Argument

    """)

add_newdoc("scipy.special", "hankel2e",
    """
    hankel2e(v, z)

    Exponentially scaled Hankel function of the second kind

    Defined as::

        hankel1e(v,z) = hankel1(v,z) * exp(1j * z)

    Parameters
    ----------
    v : float
        Order
    z : complex
        Argument
    """)

add_newdoc("scipy.special", "huber",
    r"""
    huber(delta, r)

    Huber loss function.

    .. math:: \text{huber}(\delta, r) = \begin{cases} \infty & \delta < 0  \\ \frac{1}{2}r^2 & 0 \le \delta, | r | \le \delta \\ \delta ( |r| - \frac{1}{2}\delta ) & \text{otherwise} \end{cases}

    Parameters
    ----------
    delta : ndarray
        Input array, indicating the quadratic vs. linear loss changepoint.
    r : ndarray
        Input array, possibly representing residuals.

    Returns
    -------
    res : ndarray
        The computed Huber loss function values.

    Notes
    -----
    This function is convex in r.

    .. versionadded:: 0.15.0

    """)

add_newdoc("scipy.special", "hyp1f1",
    """
    hyp1f1(a, b, x)

    Confluent hypergeometric function 1F1(a, b; x)
    """)

add_newdoc("scipy.special", "hyp1f2",
    """
    hyp1f2(a, b, c, x)

    Hypergeometric function 1F2 and error estimate

    Returns
    -------
    y
        Value of the function
    err
        Error estimate
    """)

add_newdoc("scipy.special", "hyp2f0",
    """
    hyp2f0(a, b, x, type)

    Hypergeometric function 2F0 in y and an error estimate

    The parameter `type` determines a convergence factor and can be
    either 1 or 2.

    Returns
    -------
    y
        Value of the function
    err
        Error estimate
    """)

add_newdoc("scipy.special", "hyp2f1",
    """
    hyp2f1(a, b, c, z)

    Gauss hypergeometric function 2F1(a, b; c; z).
    """)

add_newdoc("scipy.special", "hyp3f0",
    """
    hyp3f0(a, b, c, x)

    Hypergeometric function 3F0 in y and an error estimate

    Returns
    -------
    y
        Value of the function
    err
        Error estimate
    """)

add_newdoc("scipy.special", "hyperu",
    """
    hyperu(a, b, x)

    Confluent hypergeometric function U(a, b, x) of the second kind
    """)

add_newdoc("scipy.special", "i0",
    """
    i0(x)

    Modified Bessel function of order 0
    """)

add_newdoc("scipy.special", "i0e",
    """
    i0e(x)

    Exponentially scaled modified Bessel function of order 0.

    Defined as::

        i0e(x) = exp(-abs(x)) * i0(x).
    """)

add_newdoc("scipy.special", "i1",
    """
    i1(x)

    Modified Bessel function of order 1
    """)

add_newdoc("scipy.special", "i1e",
    """
    i1e(x)

    Exponentially scaled modified Bessel function of order 0.

    Defined as::

        i1e(x) = exp(-abs(x)) * i1(x)
    """)

add_newdoc("scipy.special", "it2i0k0",
    """
    it2i0k0(x)

    Integrals related to modified Bessel functions of order 0

    Returns
    -------
    ii0
        ``integral((i0(t)-1)/t, t=0..x)``
    ik0
        ``int(k0(t)/t,t=x..inf)``
    """)

add_newdoc("scipy.special", "it2j0y0",
    """
    it2j0y0(x)

    Integrals related to Bessel functions of order 0

    Returns
    -------
    ij0
        ``integral((1-j0(t))/t, t=0..x)``
    iy0
        ``integral(y0(t)/t, t=x..inf)``
    """)

add_newdoc("scipy.special", "it2struve0",
    """
    it2struve0(x)

    Integral related to Struve function of order 0

    Returns
    -------
    i
        ``integral(H0(t)/t, t=x..inf)``
    """)

add_newdoc("scipy.special", "itairy",
    """
    itairy(x)

    Integrals of Airy functios

    Calculates the integral of Airy functions from 0 to x

    Returns
    -------
    Apt, Bpt
        Integrals for positive arguments
    Ant, Bnt
        Integrals for negative arguments

    """)

add_newdoc("scipy.special", "iti0k0",
    """
    iti0k0(x)

    Integrals of modified Bessel functions of order 0

    Returns simple integrals from 0 to x of the zeroth order modified
    Bessel functions i0 and k0.

    Returns
    -------
    ii0, ik0
    """)

add_newdoc("scipy.special", "itj0y0",
    """
    itj0y0(x)

    Integrals of Bessel functions of order 0

    Returns simple integrals from 0 to x of the zeroth order Bessel
    functions j0 and y0.

    Returns
    -------
    ij0, iy0
    """)

add_newdoc("scipy.special", "itmodstruve0",
    """
    itmodstruve0(x)

    Integral of the modified Struve function of order 0

    Returns
    -------
    i
        ``integral(L0(t), t=0..x)``
    """)

add_newdoc("scipy.special", "itstruve0",
    """
    itstruve0(x)

    Integral of the Struve function of order 0

    Returns
    -------
    i
        ``integral(H0(t), t=0..x)``
    """)

add_newdoc("scipy.special", "iv",
    """
    iv(v,z)

    Modified Bessel function of the first kind  of real order

    Parameters
    ----------
    v
        Order. If z is of real type and negative, v must be integer valued.
    z
        Argument.

    """)

add_newdoc("scipy.special", "ive",
    """
    ive(v,z)

    Exponentially scaled modified Bessel function of the first kind

    Defined as::

        ive(v,z) = iv(v,z) * exp(-abs(z.real))
    """)

add_newdoc("scipy.special", "j0",
    """
    j0(x)

    Bessel function the first kind of order 0
    """)

add_newdoc("scipy.special", "j1",
    """
    j1(x)

    Bessel function of the first kind of order 1
    """)

add_newdoc("scipy.special", "jn",
    """
    jn(n, x)

    Bessel function of the first kind of integer order n.

    Notes
    -----
    `jn` is an alias of `jv`.

    """)

add_newdoc("scipy.special", "jv",
    """
    jv(v, z)

    Bessel function of the first kind of real order v
    """)

add_newdoc("scipy.special", "jve",
    """
    jve(v, z)

    Exponentially scaled Bessel function of order v

    Defined as::

        jve(v,z) = jv(v,z) * exp(-abs(z.imag))
    """)

add_newdoc("scipy.special", "k0",
    """
    k0(x)

    Modified Bessel function K of order 0

    Modified Bessel function of the second kind (sometimes called the
    third kind) of order 0.
    """)

add_newdoc("scipy.special", "k0e",
    """
    k0e(x)

    Exponentially scaled modified Bessel function K of order 0

    Defined as::

        k0e(x) = exp(x) * k0(x).
    """)

add_newdoc("scipy.special", "k1",
    """
    i1(x)

    Modified Bessel function of the first kind of order 1
    """)

add_newdoc("scipy.special", "k1e",
    """
    k1e(x)

    Exponentially scaled modified Bessel function K of order 1

    Defined as::

        k1e(x) = exp(x) * k1(x)
    """)

add_newdoc("scipy.special", "kei",
    """
    kei(x)

    Kelvin function ker
    """)

add_newdoc("scipy.special", "keip",
    """
    keip(x)

    Derivative of the Kelvin function kei
    """)

add_newdoc("scipy.special", "kelvin",
    """
    kelvin(x)

    Kelvin functions as complex numbers

    Returns
    -------
    Be, Ke, Bep, Kep
        The tuple (Be, Ke, Bep, Kep) contains complex numbers
        representing the real and imaginary Kelvin functions and their
        derivatives evaluated at x.  For example, kelvin(x)[0].real =
        ber x and kelvin(x)[0].imag = bei x with similar relationships
        for ker and kei.
    """)

add_newdoc("scipy.special", "ker",
    """
    ker(x)

    Kelvin function ker
    """)

add_newdoc("scipy.special", "kerp",
    """
    kerp(x)

    Derivative of the Kelvin function ker
    """)

add_newdoc("scipy.special", "kl_div",
    r"""
    kl_div(x, y)

    Elementwise function for computing Kullback-Leibler divergence.

    .. math:: \text{kl\_div}(x, y) = \begin{cases} x \log(x / y) - x + y & x > 0, y > 0 \\ y & x = 0, y \ge 0 \\ \infty & \text{otherwise} \end{cases}

    Parameters
    ----------
    x : ndarray
        First input array.
    y : ndarray
        Second input array.

    Returns
    -------
    res : ndarray
        Output array.

    See Also
    --------
    entr, rel_entr

    Notes
    -----
    This function is non-negative and is jointly convex in x and y.

    .. versionadded:: 0.14.0

    """)

add_newdoc("scipy.special", "kn",
    """
    kn(n, x)

    Modified Bessel function of the second kind of integer order n

    These are also sometimes called functions of the third kind.
    """)

add_newdoc("scipy.special", "kolmogi",
    """
    kolmogi(p)

    Inverse function to kolmogorov

    Returns y such that ``kolmogorov(y) == p``.
    """)

add_newdoc("scipy.special", "kolmogorov",
    """
    kolmogorov(y)

    Complementary cumulative distribution function of Kolmogorov distribution

    Returns the complementary cumulative distribution function of
    Kolmogorov's limiting distribution (Kn* for large n) of a
    two-sided test for equality between an empirical and a theoretical
    distribution. It is equal to the (limit as n->infinity of the)
    probability that sqrt(n) * max absolute deviation > y.
    """)

add_newdoc("scipy.special", "kv",
    """
    kv(v,z)

    Modified Bessel function of the second kind of real order v

    Returns the modified Bessel function of the second kind (sometimes
    called the third kind) for real order v at complex z.
    """)

add_newdoc("scipy.special", "kve",
    """
    kve(v,z)

    Exponentially scaled modified Bessel function of the second kind.

    Returns the exponentially scaled, modified Bessel function of the
    second kind (sometimes called the third kind) for real order v at
    complex z::

        kve(v,z) = kv(v,z) * exp(z)
    """)

add_newdoc("scipy.special", "log1p",
    """
    log1p(x)

    Calculates log(1+x) for use when x is near zero
    """)

add_newdoc('scipy.special', 'logit',
    """
    logit(x)

    Logit ufunc for ndarrays.

    The logit function is defined as logit(p) = log(p/(1-p)).
    Note that logit(0) = -inf, logit(1) = inf, and logit(p)
    for p<0 or p>1 yields nan.

    Parameters
    ----------
    x : ndarray
        The ndarray to apply logit to element-wise.

    Returns
    -------
    out : ndarray
        An ndarray of the same shape as x. Its entries
        are logit of the corresponding entry of x.

    Notes
    -----
    As a ufunc logit takes a number of optional
    keyword arguments. For more information
    see `ufuncs <http://docs.scipy.org/doc/numpy/reference/ufuncs.html>`_

    .. versionadded:: 0.10.0

    """)

add_newdoc("scipy.special", "lpmv",
    """
    lpmv(m, v, x)

    Associated legendre function of integer order.

    Parameters
    ----------
    m : int
        Order
    v : real
        Degree. Must be ``v>-m-1`` or ``v<m``
    x : complex
        Argument. Must be ``|x| <= 1``.

    """)

add_newdoc("scipy.special", "mathieu_a",
    """
    mathieu_a(m,q)

    Characteristic value of even Mathieu functions

    Returns the characteristic value for the even solution,
    ``ce_m(z,q)``, of Mathieu's equation.
    """)

add_newdoc("scipy.special", "mathieu_b",
    """
    mathieu_b(m,q)

    Characteristic value of odd Mathieu functions

    Returns the characteristic value for the odd solution,
    ``se_m(z,q)``, of Mathieu's equation.
    """)

add_newdoc("scipy.special", "mathieu_cem",
    """
    mathieu_cem(m,q,x)

    Even Mathieu function and its derivative

    Returns the even Mathieu function, ``ce_m(x,q)``, of order m and
    parameter q evaluated at x (given in degrees).  Also returns the
    derivative with respect to x of ce_m(x,q)

    Parameters
    ----------
    m
        Order of the function
    q
        Parameter of the function
    x
        Argument of the function, *given in degrees, not radians*

    Returns
    -------
    y
        Value of the function
    yp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "mathieu_modcem1",
    """
    mathieu_modcem1(m, q, x)

    Even modified Mathieu function of the first kind and its derivative

    Evaluates the even modified Mathieu function of the first kind,
    ``Mc1m(x,q)``, and its derivative at `x` for order m and parameter
    `q`.

    Returns
    -------
    y
        Value of the function
    yp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "mathieu_modcem2",
    """
    mathieu_modcem2(m, q, x)

    Even modified Mathieu function of the second kind and its derivative

    Evaluates the even modified Mathieu function of the second kind,
    Mc2m(x,q), and its derivative at x (given in degrees) for order m
    and parameter q.

    Returns
    -------
    y
        Value of the function
    yp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "mathieu_modsem1",
    """
    mathieu_modsem1(m,q,x)

    Odd modified Mathieu function of the first kind and its derivative

    Evaluates the odd modified Mathieu function of the first kind,
    Ms1m(x,q), and its derivative at x (given in degrees) for order m
    and parameter q.

    Returns
    -------
    y
        Value of the function
    yp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "mathieu_modsem2",
    """
    mathieu_modsem2(m, q, x)

    Odd modified Mathieu function of the second kind and its derivative

    Evaluates the odd modified Mathieu function of the second kind,
    Ms2m(x,q), and its derivative at x (given in degrees) for order m
    and parameter q.

    Returns
    -------
    y
        Value of the function
    yp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "mathieu_sem",
    """
    mathieu_sem(m, q, x)

    Odd Mathieu function and its derivative

    Returns the odd Mathieu function, se_m(x,q), of order m and
    parameter q evaluated at x (given in degrees).  Also returns the
    derivative with respect to x of se_m(x,q).

    Parameters
    ----------
    m
        Order of the function
    q
        Parameter of the function
    x
        Argument of the function, *given in degrees, not radians*.

    Returns
    -------
    y
        Value of the function
    yp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "modfresnelm",
    """
    modfresnelm(x)

    Modified Fresnel negative integrals

    Returns
    -------
    fm
        Integral ``F_-(x)``: ``integral(exp(-1j*t*t),t=x..inf)``
    km
        Integral ``K_-(x)``: ``1/sqrt(pi)*exp(1j*(x*x+pi/4))*fp``
    """)

add_newdoc("scipy.special", "modfresnelp",
    """
    modfresnelp(x)

    Modified Fresnel positive integrals

    Returns
    -------
    fp
        Integral ``F_+(x)``: ``integral(exp(1j*t*t),t=x..inf)``
    kp
        Integral ``K_+(x)``: ``1/sqrt(pi)*exp(-1j*(x*x+pi/4))*fp``
    """)

add_newdoc("scipy.special", "modstruve",
    """
    modstruve(v, x)

    Modified Struve function

    Returns the modified Struve function Lv(x) of order v at x, x must
    be positive unless v is an integer.
    """)

add_newdoc("scipy.special", "nbdtr",
    """
    nbdtr(k, n, p)

    Negative binomial cumulative distribution function

    Returns the sum of the terms 0 through k of the negative binomial
    distribution::

        sum((n+j-1)Cj p**n (1-p)**j,j=0..k).

    In a sequence of Bernoulli trials this is the probability that k
    or fewer failures precede the nth success.
    """)

add_newdoc("scipy.special", "nbdtrc",
    """
    nbdtrc(k,n,p)

    Negative binomial survival function

    Returns the sum of the terms k+1 to infinity of the negative
    binomial distribution.
    """)

add_newdoc("scipy.special", "nbdtri",
    """
    nbdtri(k, n, y)

    Inverse of nbdtr vs p

    Finds the argument p such that ``nbdtr(k,n,p) = y``.
    """)

add_newdoc("scipy.special", "nbdtrik",
    """
    nbdtrik(y,n,p)

    Inverse of nbdtr vs k

    Finds the argument k such that ``nbdtr(k,n,p) = y``.
    """)

add_newdoc("scipy.special", "nbdtrin",
    """
    nbdtrin(k,y,p)

    Inverse of nbdtr vs n

    Finds the argument n such that ``nbdtr(k,n,p) = y``.
    """)

add_newdoc("scipy.special", "ncfdtr",
    """
    ncfdtr(dfn, dfd, nc, f)

    Cumulative distribution function of the non-central F distribution.

    Parameters
    ----------
    dfn : array_like
        Degrees of freedom of the numerator sum of squares.  Range (0, inf).
    dfd : array_like
        Degrees of freedom of the denominator sum of squares.  Range (0, inf).
    nc : array_like
        Noncentrality parameter.  Should be in range (0, 1e4).
    f : array_like
        Quantiles, i.e. the upper limit of integration.

    Returns
    -------
    cdf : float or ndarray
        The calculated CDF.  If all inputs are scalar, the return will be a
        float.  Otherwise it will be an array.

    See Also
    --------
    ncdfdtri : Inverse CDF (iCDF) of the non-central F distribution.
    ncdfdtridfd : Calculate dfd, given CDF and iCDF values.
    ncdfdtridfn : Calculate dfn, given CDF and iCDF values.
    ncdfdtrinc : Calculate noncentrality parameter, given CDF, iCDF, dfn, dfd.

    Examples
    --------
    >>> from scipy import special
    >>> from scipy import stats
    >>> import matplotlib.pyplot as plt

    Plot the CDF of the non-central F distribution, for nc=0.  Compare with the
    F-distribution from scipy.stats:

    >>> x = np.linspace(-1, 8, num=500)
    >>> dfn = 3
    >>> dfd = 2
    >>> ncf_stats = stats.f.cdf(x, dfn, dfd)
    >>> ncf_special = special.ncfdtr(dfn, dfd, 0, x)

    >>> fig = plt.figure()
    >>> ax = fig.add_subplot(111)
    >>> ax.plot(x, ncf_stats, 'b-', lw=3)
    >>> ax.plot(x, ncf_special, 'r-')
    >>> plt.show()

    """)

add_newdoc("scipy.special", "ncfdtri",
    """
    ncfdtri(p, dfn, dfd, nc)

    Inverse cumulative distribution function of the non-central F distribution.

    See `ncfdtr` for more details.

    """)

add_newdoc("scipy.special", "ncfdtridfd",
    """
    ncfdtridfd(p, f, dfn, nc)

    Calculate degrees of freedom (denominator) for the noncentral F-distribution.

    See `ncfdtr` for more details.

    """)

add_newdoc("scipy.special", "ncfdtridfn",
    """
    ncfdtridfn(p, f, dfd, nc)

    Calculate degrees of freedom (numerator) for the noncentral F-distribution.

    See `ncfdtr` for more details.

    """)

add_newdoc("scipy.special", "ncfdtrinc",
    """
    ncfdtrinc(p, f, dfn, dfd)

    Calculate non-centrality parameter for non-central F distribution.

    See `ncfdtr` for more details.

    """)

add_newdoc("scipy.special", "nctdtr",
    """
    nctdtr(df, nc, t)

    Cumulative distribution function of the non-central t distribution.

    Parameters
    ----------
    df : array_like
        Degrees of freedom of the distribution.  Should be in range (0, inf).
    nc : array_like
        Noncentrality parameter.  Should be in range (-1e6, 1e6).
    t : array_like
        Quantiles, i.e. the upper limit of integration.

    Returns
    -------
    cdf : float or ndarray
        The calculated CDF.  If all inputs are scalar, the return will be a
        float.  Otherwise it will be an array.

    See Also
    --------
    nctdtrit : Inverse CDF (iCDF) of the non-central t distribution.
    nctdtridf : Calculate degrees of freedom, given CDF and iCDF values.
    nctdtrinc : Calculate non-centrality parameter, given CDF iCDF values.

    Examples
    --------
    >>> from scipy import special
    >>> from scipy import stats
    >>> import matplotlib.pyplot as plt

    Plot the CDF of the non-central t distribution, for nc=0.  Compare with the
    t-distribution from scipy.stats:

    >>> x = np.linspace(-5, 5, num=500)
    >>> df = 3
    >>> nct_stats = stats.t.cdf(x, df)
    >>> nct_special = special.nctdtr(df, 0, x)

    >>> fig = plt.figure()
    >>> ax = fig.add_subplot(111)
    >>> ax.plot(x, nct_stats, 'b-', lw=3)
    >>> ax.plot(x, nct_special, 'r-')
    >>> plt.show()

    """)

add_newdoc("scipy.special", "nctdtridf",
    """
    nctdtridf(p, nc, t)

    Calculate degrees of freedom for non-central t distribution.

    See `nctdtr` for more details.

    Parameters
    ----------
    p : array_like
        CDF values, in range (0, 1].
    nc : array_like
        Noncentrality parameter.  Should be in range (-1e6, 1e6).
    t : array_like
        Quantiles, i.e. the upper limit of integration.

    """)

add_newdoc("scipy.special", "nctdtrinc",
    """
    nctdtrinc(df, p, t)

    Calculate non-centrality parameter for non-central t distribution.

    See `nctdtr` for more details.

    Parameters
    ----------
    df : array_like
        Degrees of freedom of the distribution.  Should be in range (0, inf).
    p : array_like
        CDF values, in range (0, 1].
    t : array_like
        Quantiles, i.e. the upper limit of integration.

    """)

add_newdoc("scipy.special", "nctdtrit",
    """
    nctdtrit(df, nc, p)

    Inverse cumulative distribution function of the non-central t distribution.

    See `nctdtr` for more details.

    Parameters
    ----------
    df : array_like
        Degrees of freedom of the distribution.  Should be in range (0, inf).
    nc : array_like
        Noncentrality parameter.  Should be in range (-1e6, 1e6).
    p : array_like
        CDF values, in range (0, 1].

    """)

add_newdoc("scipy.special", "ndtr",
    """
    ndtr(x)

    Gaussian cumulative distribution function

    Returns the area under the standard Gaussian probability
    density function, integrated from minus infinity to x::

        1/sqrt(2*pi) * integral(exp(-t**2 / 2),t=-inf..x)

    """)

add_newdoc("scipy.special", "nrdtrimn",
    """
    nrdtrimn(p, x, std)

    Calculate mean of normal distribution given other params.

    Parameters
    ----------
    p : array_like
        CDF values, in range (0, 1].
    x : array_like
        Quantiles, i.e. the upper limit of integration.
    std : array_like
        Standard deviation.

    Returns
    -------
    mn : float or ndarray
        The mean of the normal distribution.

    See Also
    --------
    nrdtrimn, ndtr

    """)

add_newdoc("scipy.special", "nrdtrisd",
    """
    nrdtrisd(p, x, mn)

    Calculate standard deviation of normal distribution given other params.

    Parameters
    ----------
    p : array_like
        CDF values, in range (0, 1].
    x : array_like
        Quantiles, i.e. the upper limit of integration.
    mn : float or ndarray
        The mean of the normal distribution.

    Returns
    -------
    std : array_like
        Standard deviation.

    See Also
    --------
    nrdtristd, ndtr

    """)

add_newdoc("scipy.special", "log_ndtr",
    """
    log_ndtr(x)

    Logarithm of Gaussian cumulative distribution function

    Returns the log of the area under the standard Gaussian probability
    density function, integrated from minus infinity to x::

        log(1/sqrt(2*pi) * integral(exp(-t**2 / 2), t=-inf..x))
    """)

add_newdoc("scipy.special", "ndtri",
    """
    ndtri(y)

    Inverse of ndtr vs x

    Returns the argument x for which the area under the Gaussian
    probability density function (integrated from minus infinity to x)
    is equal to y.
    """)

add_newdoc("scipy.special", "obl_ang1",
    """
    obl_ang1(m, n, c, x)

    Oblate spheroidal angular function of the first kind and its derivative

    Computes the oblate spheroidal angular function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "obl_ang1_cv",
    """
    obl_ang1_cv(m, n, c, cv, x)

    Oblate spheroidal angular function obl_ang1 for precomputed characteristic value

    Computes the oblate spheroidal angular function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``. Requires
    pre-computed characteristic value.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "obl_cv",
    """
    obl_cv(m, n, c)

    Characteristic value of oblate spheroidal function

    Computes the characteristic value of oblate spheroidal wave
    functions of order m,n (n>=m) and spheroidal parameter c.
    """)

add_newdoc("scipy.special", "obl_rad1",
    """
    obl_rad1(m,n,c,x)

    Oblate spheroidal radial function of the first kind and its derivative

    Computes the oblate spheroidal radial function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "obl_rad1_cv",
    """
    obl_rad1_cv(m,n,c,cv,x)

    Oblate spheroidal radial function obl_rad1 for precomputed characteristic value

    Computes the oblate spheroidal radial function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``. Requires
    pre-computed characteristic value.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "obl_rad2",
    """
    obl_rad2(m,n,c,x)

    Oblate spheroidal radial function of the second kind and its derivative.

    Computes the oblate spheroidal radial function of the second kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "obl_rad2_cv",
    """
    obl_rad2_cv(m,n,c,cv,x)

    Oblate spheroidal radial function obl_rad2 for precomputed characteristic value

    Computes the oblate spheroidal radial function of the second kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``. Requires
    pre-computed characteristic value.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pbdv",
    """
    pbdv(v, x)

    Parabolic cylinder function D

    Returns (d,dp) the parabolic cylinder function Dv(x) in d and the
    derivative, Dv'(x) in dp.

    Returns
    -------
    d
        Value of the function
    dp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pbvv",
    """
    pbvv(v,x)

    Parabolic cylinder function V

    Returns the parabolic cylinder function Vv(x) in v and the
    derivative, Vv'(x) in vp.

    Returns
    -------
    v
        Value of the function
    vp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pbwa",
    """
    pbwa(a,x)

    Parabolic cylinder function W

    Returns the parabolic cylinder function W(a,x) in w and the
    derivative, W'(a,x) in wp.

    .. warning::

       May not be accurate for large (>5) arguments in a and/or x.

    Returns
    -------
    w
        Value of the function
    wp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pdtr",
    """
    pdtr(k, m)

    Poisson cumulative distribution function

    Returns the sum of the first k terms of the Poisson distribution:
    sum(exp(-m) * m**j / j!, j=0..k) = gammaincc( k+1, m).  Arguments
    must both be positive and k an integer.
    """)

add_newdoc("scipy.special", "pdtrc",
    """
    pdtrc(k, m)

    Poisson survival function

    Returns the sum of the terms from k+1 to infinity of the Poisson
    distribution: sum(exp(-m) * m**j / j!, j=k+1..inf) = gammainc(
    k+1, m).  Arguments must both be positive and k an integer.
    """)

add_newdoc("scipy.special", "pdtri",
    """
    pdtri(k,y)

    Inverse to pdtr vs m

    Returns the Poisson variable m such that the sum from 0 to k of
    the Poisson density is equal to the given probability y:
    calculated by gammaincinv(k+1, y).  k must be a nonnegative
    integer and y between 0 and 1.
    """)

add_newdoc("scipy.special", "pdtrik",
    """
    pdtrik(p,m)

    Inverse to pdtr vs k

    Returns the quantile k such that ``pdtr(k, m) = p``
    """)

add_newdoc("scipy.special", "poch",
    """
    poch(z, m)

    Rising factorial (z)_m

    The Pochhammer symbol (rising factorial), is defined as::

        (z)_m = gamma(z + m) / gamma(z)

    For positive integer `m` it reads::

        (z)_m = z * (z + 1) * ... * (z + m - 1)
    """)

add_newdoc("scipy.special", "pro_ang1",
    """
    pro_ang1(m,n,c,x)

    Prolate spheroidal angular function of the first kind and its derivative

    Computes the prolate spheroidal angular function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pro_ang1_cv",
    """
    pro_ang1_cv(m,n,c,cv,x)

    Prolate spheroidal angular function pro_ang1 for precomputed characteristic value

    Computes the prolate spheroidal angular function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``. Requires
    pre-computed characteristic value.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pro_cv",
    """
    pro_cv(m,n,c)

    Characteristic value of prolate spheroidal function

    Computes the characteristic value of prolate spheroidal wave
    functions of order m,n (n>=m) and spheroidal parameter c.
    """)

add_newdoc("scipy.special", "pro_rad1",
    """
    pro_rad1(m,n,c,x)

    Prolate spheroidal radial function of the first kind and its derivative

    Computes the prolate spheroidal radial function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pro_rad1_cv",
    """
    pro_rad1_cv(m,n,c,cv,x)

    Prolate spheroidal radial function pro_rad1 for precomputed characteristic value

    Computes the prolate spheroidal radial function of the first kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``. Requires
    pre-computed characteristic value.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pro_rad2",
    """
    pro_rad2(m,n,c,x)

    Prolate spheroidal radial function of the secon kind and its derivative

    Computes the prolate spheroidal radial function of the second kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pro_rad2_cv",
    """
    pro_rad2_cv(m,n,c,cv,x)

    Prolate spheroidal radial function pro_rad2 for precomputed characteristic value

    Computes the prolate spheroidal radial function of the second kind
    and its derivative (with respect to x) for mode parameters m>=0
    and n>=m, spheroidal parameter c and ``|x| < 1.0``. Requires
    pre-computed characteristic value.

    Returns
    -------
    s
        Value of the function
    sp
        Value of the derivative vs x
    """)

add_newdoc("scipy.special", "pseudo_huber",
    r"""
    pseudo_huber(delta, r)

    Pseudo-Huber loss function.

    .. math:: \text{pseudo\_huber}(\delta, r) = \delta^2 \left( \sqrt{ 1 + \left( \frac{r}{\delta} \right)^2 } - 1 \right)

    Parameters
    ----------
    delta : ndarray
        Input array, indicating the soft quadratic vs. linear loss changepoint.
    r : ndarray
        Input array, possibly representing residuals.

    Returns
    -------
    res : ndarray
        The computed Pseudo-Huber loss function values.

    Notes
    -----
    This function is convex in r.

    .. versionadded:: 0.15.0

    """)

add_newdoc("scipy.special", "psi",
    """
    psi(z)

    Digamma function

    The derivative of the logarithm of the gamma function evaluated at
    z (also called the digamma function).
    """)

add_newdoc("scipy.special", "radian",
    """
    radian(d, m, s)

    Convert from degrees to radians

    Returns the angle given in (d)egrees, (m)inutes, and (s)econds in
    radians.
    """)

add_newdoc("scipy.special", "rel_entr",
    r"""
    rel_entr(x, y)

    Elementwise function for computing relative entropy.

    .. math:: \text{rel\_entr}(x, y) = \begin{cases} x \log(x / y) & x > 0, y > 0 \\ 0 & x = 0, y \ge 0 \\ \infty & \text{otherwise} \end{cases}

    Parameters
    ----------
    x : ndarray
        First input array.
    y : ndarray
        Second input array.

    Returns
    -------
    res : ndarray
        Output array.

    See Also
    --------
    entr, kl_div

    Notes
    -----
    This function is jointly convex in x and y.

    .. versionadded:: 0.14.0

    """)

add_newdoc("scipy.special", "rgamma",
    """
    rgamma(z)

    Gamma function inverted

    Returns ``1/gamma(x)``
    """)

add_newdoc("scipy.special", "round",
    """
    round(x)

    Round to nearest integer

    Returns the nearest integer to x as a double precision floating
    point result.  If x ends in 0.5 exactly, the nearest even integer
    is chosen.
    """)

add_newdoc("scipy.special", "shichi",
    """
    shichi(x)

    Hyperbolic sine and cosine integrals

    Returns
    -------
    shi
        ``integral(sinh(t)/t, t=0..x)``
    chi
        ``eul + ln x + integral((cosh(t)-1)/t, t=0..x)``
        where ``eul`` is Euler's constant.
    """)

add_newdoc("scipy.special", "sici",
    """
    sici(x)

    Sine and cosine integrals

    Returns
    -------
    si
        ``integral(sin(t)/t, t=0..x)``
    ci
        ``eul + ln x + integral((cos(t) - 1)/t, t=0..x)``
        where ``eul`` is Euler's constant.
    """)

add_newdoc("scipy.special", "sindg",
    """
    sindg(x)

    Sine of angle given in degrees
    """)

add_newdoc("scipy.special", "smirnov",
    """
    smirnov(n, e)

    Kolmogorov-Smirnov complementary cumulative distribution function

    Returns the exact Kolmogorov-Smirnov complementary cumulative
    distribution function (Dn+ or Dn-) for a one-sided test of
    equality between an empirical and a theoretical distribution. It
    is equal to the probability that the maximum difference between a
    theoretical distribution and an empirical one based on n samples
    is greater than e.
    """)

add_newdoc("scipy.special", "smirnovi",
    """
    smirnovi(n, y)

    Inverse to smirnov

    Returns ``e`` such that ``smirnov(n, e) = y``.
    """)

add_newdoc("scipy.special", "spence",
    """
    spence(x)

    Dilogarithm integral

    Returns the dilogarithm integral::

        -integral(log t / (t-1),t=1..x)
    """)

add_newdoc("scipy.special", "stdtr",
    """
    stdtr(df,t)

    Student t distribution cumulative density function

    Returns the integral from minus infinity to t of the Student t
    distribution with df > 0 degrees of freedom::

       gamma((df+1)/2)/(sqrt(df*pi)*gamma(df/2)) *
       integral((1+x**2/df)**(-df/2-1/2), x=-inf..t)

    """)

add_newdoc("scipy.special", "stdtridf",
    """
    stdtridf(p,t)

    Inverse of stdtr vs df

    Returns the argument df such that stdtr(df,t) is equal to p.
    """)

add_newdoc("scipy.special", "stdtrit",
    """
    stdtrit(df,p)

    Inverse of stdtr vs t

    Returns the argument t such that stdtr(df,t) is equal to p.
    """)

add_newdoc("scipy.special", "struve",
    """
    struve(v,x)

    Struve function

    Computes the struve function Hv(x) of order v at x, x must be
    positive unless v is an integer.
    """)

add_newdoc("scipy.special", "tandg",
    """
    tandg(x)

    Tangent of angle x given in degrees.
    """)

add_newdoc("scipy.special", "tklmbda",
    """
    tklmbda(x, lmbda)

    Tukey-Lambda cumulative distribution function

    """)

add_newdoc("scipy.special", "wofz",
    """
    wofz(z)

    Faddeeva function

    Returns the value of the Faddeeva function for complex argument::

        exp(-z**2)*erfc(-i*z)

    References
    ----------
    .. [1] Steven G. Johnson, Faddeeva W function implementation.
       http://ab-initio.mit.edu/Faddeeva
    """)

add_newdoc("scipy.special", "xlogy",
    """
    xlogy(x, y)

    Compute ``x*log(y)`` so that the result is 0 if `x = 0`.

    Parameters
    ----------
    x : array_like
        Multiplier
    y : array_like
        Argument

    Returns
    -------
    z : array_like
        Computed x*log(y)

    Notes
    -----

    .. versionadded:: 0.13.0

    """)

add_newdoc("scipy.special", "xlog1py",
    """
    xlog1py(x, y)

    Compute ``x*log1p(y)`` so that the result is 0 if `x = 0`.

    Parameters
    ----------
    x : array_like
        Multiplier
    y : array_like
        Argument

    Returns
    -------
    z : array_like
        Computed x*log1p(y)

    Notes
    -----

    .. versionadded:: 0.13.0

    """)

add_newdoc("scipy.special", "y0",
    """
    y0(x)

    Bessel function of the second kind of order 0

    Returns the Bessel function of the second kind of order 0 at x.
    """)

add_newdoc("scipy.special", "y1",
    """
    y1(x)

    Bessel function of the second kind of order 1

    Returns the Bessel function of the second kind of order 1 at x.
    """)

add_newdoc("scipy.special", "yn",
    """
    yn(n,x)

    Bessel function of the second kind of integer order

    Returns the Bessel function of the second kind of integer order n
    at x.
    """)

add_newdoc("scipy.special", "yv",
    """
    yv(v,z)

    Bessel function of the second kind of real order

    Returns the Bessel function of the second kind of real order v at
    complex z.
    """)

add_newdoc("scipy.special", "yve",
    """
    yve(v,z)

    Exponentially scaled Bessel function of the second kind of real order

    Returns the exponentially scaled Bessel function of the second
    kind of real order v at complex z::

        yve(v,z) = yv(v,z) * exp(-abs(z.imag))

    """)

add_newdoc("scipy.special", "zeta",
    """
    zeta(x, q)

    Hurwitz zeta function

    The Riemann zeta function of two arguments (also known as the
    Hurwitz zeta funtion).

    This function is defined as

    .. math:: \\zeta(x, q) = \\sum_{k=0}^{\\infty} 1 / (k+q)^x,

    where ``x > 1`` and ``q > 0``.

    See also
    --------
    zetac

    """)

add_newdoc("scipy.special", "zetac",
    """
    zetac(x)

    Riemann zeta function minus 1.

    This function is defined as

    .. math:: \\zeta(x) = \\sum_{k=2}^{\\infty} 1 / k^x,

    where ``x > 1``.

    See Also
    --------
    zeta

    """)

add_newdoc("scipy.special", "_struve_asymp_large_z",
    """
    _struve_asymp_large_z(v, z, is_h)

    Internal function for testing struve & modstruve

    Evaluates using asymptotic expansion

    Returns
    -------
    v, err
    """)

add_newdoc("scipy.special", "_struve_power_series",
    """
    _struve_power_series(v, z, is_h)

    Internal function for testing struve & modstruve

    Evaluates using power series

    Returns
    -------
    v, err
    """)

add_newdoc("scipy.special", "_struve_bessel_series",
    """
    _struve_bessel_series(v, z, is_h)

    Internal function for testing struve & modstruve

    Evaluates using Bessel function series

    Returns
    -------
    v, err
    """)
