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# scipy.special.gdtrix

scipy.special.gdtrix(a, b, p, out=None) = <ufunc 'gdtrix'>

  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 pth 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 scalar or 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).

  Notes

  Wrapper for the CDFLIB [1] Fortran routine cdfgam.

  The cumulative distribution function p is computed using a routine by DiDinato and Morris [2]. Computation of x involves a search for a value that produces the desired value of p. The search relies on the monotonicity of p with x.

  References

  [1]

  Barry Brown, James Lovato, and Kathy Russell, CDFLIB: Library of Fortran Routines for Cumulative Distribution Functions, Inverses, and Other Parameters.

  [2]

  DiDinato, A. R. and Morris, A. H., Computation of the incomplete gamma function ratios and their inverse. ACM Trans. Math. Softw. 12 (1986), 377-393.

  Examples

  First evaluate `gdtr`.

      >>> from scipy.special import gdtr, gdtrix
      >>> p = gdtr(1.2, 3.4, 5.6)
      >>> print(p)
      0.94378087442

  Verify the inverse.

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