"""
Support and standalone functions for Robust Linear Models
References
----------
PJ Huber. 'Robust Statistics' John Wiley and Sons, Inc., New York, 1981.
R Venables, B Ripley. 'Modern Applied Statistics in S'
Springer, New York, 2002.
"""
from statsmodels.compat.python import callable, range
import numpy as np
from scipy.stats import norm as Gaussian
from . import norms
from statsmodels.tools import tools
[docs]def mad(a, c=Gaussian.ppf(3/4.), axis=0, center=np.median):
# c \approx .6745
"""
The Median Absolute Deviation along given axis of an array
Parameters
----------
a : array-like
Input array.
c : float, optional
The normalization constant. Defined as scipy.stats.norm.ppf(3/4.),
which is approximately .6745.
axis : int, optional
The defaul is 0. Can also be None.
center : callable or float
If a callable is provided, such as the default `np.median` then it
is expected to be called center(a). The axis argument will be applied
via np.apply_over_axes. Otherwise, provide a float.
Returns
-------
mad : float
`mad` = median(abs(`a` - center))/`c`
"""
a = np.asarray(a)
if callable(center):
center = np.apply_over_axes(center, a, axis)
return np.median((np.fabs(a-center))/c, axis=axis)
[docs]class Huber(object):
"""
Huber's proposal 2 for estimating location and scale jointly.
Parameters
----------
c : float, optional
Threshold used in threshold for chi=psi**2. Default value is 1.5.
tol : float, optional
Tolerance for convergence. Default value is 1e-08.
maxiter : int, optional0
Maximum number of iterations. Default value is 30.
norm : statsmodels.robust.norms.RobustNorm, optional
A robust norm used in M estimator of location. If None,
the location estimator defaults to a one-step
fixed point version of the M-estimator using Huber's T.
call
Return joint estimates of Huber's scale and location.
Examples
--------
>>> import numpy as np
>>> import statsmodels.api as sm
>>> chem_data = np.array([2.20, 2.20, 2.4, 2.4, 2.5, 2.7, 2.8, 2.9, 3.03,
... 3.03, 3.10, 3.37, 3.4, 3.4, 3.4, 3.5, 3.6, 3.7, 3.7, 3.7, 3.7,
... 3.77, 5.28, 28.95])
>>> sm.robust.scale.huber(chem_data)
(array(3.2054980819923693), array(0.67365260010478967))
"""
def __init__(self, c=1.5, tol=1.0e-08, maxiter=30, norm=None):
self.c = c
self.maxiter = maxiter
self.tol = tol
self.norm = norm
tmp = 2 * Gaussian.cdf(c) - 1
self.gamma = tmp + c**2 * (1 - tmp) - 2 * c * Gaussian.pdf(c)
def __call__(self, a, mu=None, initscale=None, axis=0):
"""
Compute Huber's proposal 2 estimate of scale, using an optional
initial value of scale and an optional estimate of mu. If mu
is supplied, it is not reestimated.
Parameters
----------
a : array
1d array
mu : float or None, optional
If the location mu is supplied then it is not reestimated.
Default is None, which means that it is estimated.
initscale : float or None, optional
A first guess on scale. If initscale is None then the standardized
median absolute deviation of a is used.
Notes
-----
`Huber` minimizes the function
sum(psi((a[i]-mu)/scale)**2)
as a function of (mu, scale), where
psi(x) = np.clip(x, -self.c, self.c)
"""
a = np.asarray(a)
if mu is None:
n = a.shape[0] - 1
mu = np.median(a, axis=axis)
est_mu = True
else:
n = a.shape[0]
mu = mu
est_mu = False
if initscale is None:
scale = mad(a, axis=axis)
else:
scale = initscale
scale = tools.unsqueeze(scale, axis, a.shape)
mu = tools.unsqueeze(mu, axis, a.shape)
return self._estimate_both(a, scale, mu, axis, est_mu, n)
def _estimate_both(self, a, scale, mu, axis, est_mu, n):
"""
Estimate scale and location simultaneously with the following
pseudo_loop:
while not_converged:
mu, scale = estimate_location(a, scale, mu), estimate_scale(a, scale, mu)
where estimate_location is an M-estimator and estimate_scale implements
the check used in Section 5.5 of Venables & Ripley
"""
for _ in range(self.maxiter):
# Estimate the mean along a given axis
if est_mu:
if self.norm is None:
# This is a one-step fixed-point estimator
# if self.norm == norms.HuberT
# It should be faster than using norms.HuberT
nmu = np.clip(a, mu-self.c*scale,
mu+self.c*scale).sum(axis) / a.shape[axis]
else:
nmu = norms.estimate_location(a, scale, self.norm, axis, mu,
self.maxiter, self.tol)
else:
# Effectively, do nothing
nmu = mu.squeeze()
nmu = tools.unsqueeze(nmu, axis, a.shape)
subset = np.less_equal(np.fabs((a - mu)/scale), self.c)
card = subset.sum(axis)
nscale = np.sqrt(np.sum(subset * (a - nmu)**2, axis) \
/ (n * self.gamma - (a.shape[axis] - card) * self.c**2))
nscale = tools.unsqueeze(nscale, axis, a.shape)
test1 = np.alltrue(np.less_equal(np.fabs(scale - nscale),
nscale * self.tol))
test2 = np.alltrue(np.less_equal(np.fabs(mu - nmu), nscale*self.tol))
if not (test1 and test2):
mu = nmu; scale = nscale
else:
return nmu.squeeze(), nscale.squeeze()
raise ValueError('joint estimation of location and scale failed to converge in %d iterations' % self.maxiter)
huber = Huber()
[docs]class HuberScale(object):
"""
Huber's scaling for fitting robust linear models.
Huber's scale is intended to be used as the scale estimate in the
IRLS algorithm and is slightly different than the `Huber` class.
Parameters
----------
d : float, optional
d is the tuning constant for Huber's scale. Default is 2.5
tol : float, optional
The convergence tolerance
maxiter : int, optiona
The maximum number of iterations. The default is 30.
Methods
-------
call
Return's Huber's scale computed as below
Notes
--------
Huber's scale is the iterative solution to
scale_(i+1)**2 = 1/(n*h)*sum(chi(r/sigma_i)*sigma_i**2
where the Huber function is
chi(x) = (x**2)/2 for \|x\| < d
chi(x) = (d**2)/2 for \|x\| >= d
and the Huber constant h = (n-p)/n*(d**2 + (1-d**2)*\
scipy.stats.norm.cdf(d) - .5 - d*sqrt(2*pi)*exp(-0.5*d**2)
"""
def __init__(self, d=2.5, tol=1e-08, maxiter=30):
self.d = d
self.tol = tol
self.maxiter = maxiter
def __call__(self, df_resid, nobs, resid):
h = (df_resid)/nobs*(self.d**2 + (1-self.d**2)*\
Gaussian.cdf(self.d)-.5 - self.d/(np.sqrt(2*np.pi))*\
np.exp(-.5*self.d**2))
s = mad(resid)
subset = lambda x: np.less(np.fabs(resid/x),self.d)
chi = lambda s: subset(s)*(resid/s)**2/2+(1-subset(s))*(self.d**2/2)
scalehist = [np.inf,s]
niter = 1
while (np.abs(scalehist[niter-1] - scalehist[niter])>self.tol \
and niter < self.maxiter):
nscale = np.sqrt(1/(nobs*h)*np.sum(chi(scalehist[-1]))*\
scalehist[-1]**2)
scalehist.append(nscale)
niter += 1
#if niter == self.maxiter:
# raise ValueError("Huber's scale failed to converge")
return scalehist[-1]
hubers_scale = HuberScale()
