Kernel Density Estimation#
Kernel density estimation is the process of estimating an unknown probability density function using a kernel function \(K(u)\). While a histogram counts the number of data points in somewhat arbitrary regions, a kernel density estimate is a function defined as the sum of a kernel function on every data point. The kernel function typically exhibits the following properties:
Symmetry such that \(K(u) = K(-u)\).
Normalization such that \(\int_{-\infty}^{\infty} K(u) \ du = 1\) .
Monotonically decreasing such that \(K'(u) < 0\) when \(u > 0\).
Expected value equal to zero such that \(\mathrm{E}[K] = 0\).
For more information about kernel density estimation, see for instance Wikipedia - Kernel density estimation.
A univariate kernel density estimator is implemented in sm.nonparametric.KDEUnivariate. In this example we will show the following:
Basic usage, how to fit the estimator.
The effect of varying the bandwidth of the kernel using the
bwargument.The various kernel functions available using the
kernelargument.
[1]:
%matplotlib inline
import matplotlib.pyplot as plt
import numpy as np
from scipy import stats
import statsmodels.api as sm
from statsmodels.distributions.mixture_rvs import mixture_rvs
A univariate example#
[2]:
np.random.seed(12345) # Seed the random number generator for reproducible results
We create a bimodal distribution: a mixture of two normal distributions with locations at -1 and 1.
[3]:
# Location, scale and weight for the two distributions
dist1_loc, dist1_scale, weight1 = -1, 0.5, 0.25
dist2_loc, dist2_scale, weight2 = 1, 0.5, 0.75
# Sample from a mixture of distributions
obs_dist = mixture_rvs(
prob=[weight1, weight2],
size=250,
dist=[stats.norm, stats.norm],
kwargs=(
dict(loc=dist1_loc, scale=dist1_scale),
dict(loc=dist2_loc, scale=dist2_scale),
),
)
The simplest non-parametric technique for density estimation is the histogram.
[4]:
fig = plt.figure(figsize=(12, 5))
ax = fig.add_subplot(111)
# Scatter plot of data samples and histogram
ax.scatter(
obs_dist,
np.abs(np.random.randn(obs_dist.size)),
zorder=15,
color="red",
marker="x",
alpha=0.5,
label="Samples",
)
lines = ax.hist(obs_dist, bins=20, edgecolor="k", label="Histogram")
ax.legend(loc="best")
ax.grid(True, zorder=-5)
Fitting with the default arguments#
The histogram above is discontinuous. To compute a continuous probability density function, we can use kernel density estimation.
We initialize a univariate kernel density estimator using KDEUnivariate.
[5]:
kde = sm.nonparametric.KDEUnivariate(obs_dist)
kde.fit() # Estimate the densities
[5]:
<statsmodels.nonparametric.kde.KDEUnivariate at 0x7f9cc6caa3c0>
We present a figure of the fit, as well as the true distribution.
[6]:
fig = plt.figure(figsize=(12, 5))
ax = fig.add_subplot(111)
# Plot the histogram
ax.hist(
obs_dist,
bins=20,
density=True,
label="Histogram from samples",
zorder=5,
edgecolor="k",
alpha=0.5,
)
# Plot the KDE as fitted using the default arguments
ax.plot(kde.support, kde.density, lw=3, label="KDE from samples", zorder=10)
# Plot the true distribution
true_values = (
stats.norm.pdf(loc=dist1_loc, scale=dist1_scale, x=kde.support) * weight1
+ stats.norm.pdf(loc=dist2_loc, scale=dist2_scale, x=kde.support) * weight2
)
ax.plot(kde.support, true_values, lw=3, label="True distribution", zorder=15)
# Plot the samples
ax.scatter(
obs_dist,
np.abs(np.random.randn(obs_dist.size)) / 40,
marker="x",
color="red",
zorder=20,
label="Samples",
alpha=0.5,
)
ax.legend(loc="best")
ax.grid(True, zorder=-5)
In the code above, default arguments were used. We can also vary the bandwidth of the kernel, as we will now see.
Varying the bandwidth using the bw argument#
The bandwidth of the kernel can be adjusted using the bw argument. In the following example, a bandwidth of bw=0.2 seems to fit the data well.
[7]:
fig = plt.figure(figsize=(12, 5))
ax = fig.add_subplot(111)
# Plot the histogram
ax.hist(
obs_dist,
bins=25,
label="Histogram from samples",
zorder=5,
edgecolor="k",
density=True,
alpha=0.5,
)
# Plot the KDE for various bandwidths
for bandwidth in [0.1, 0.2, 0.4]:
kde.fit(bw=bandwidth) # Estimate the densities
ax.plot(
kde.support,
kde.density,
"--",
lw=2,
color="k",
zorder=10,
label="KDE from samples, bw = {}".format(round(bandwidth, 2)),
)
# Plot the true distribution
ax.plot(kde.support, true_values, lw=3, label="True distribution", zorder=15)
# Plot the samples
ax.scatter(
obs_dist,
np.abs(np.random.randn(obs_dist.size)) / 50,
marker="x",
color="red",
zorder=20,
label="Data samples",
alpha=0.5,
)
ax.legend(loc="best")
ax.set_xlim([-3, 3])
ax.grid(True, zorder=-5)
Comparing kernel functions#
In the example above, a Gaussian kernel was used. Several other kernels are also available.
[8]:
from statsmodels.nonparametric.kde import kernel_switch
list(kernel_switch.keys())
[8]:
['gau', 'epa', 'uni', 'tri', 'biw', 'triw', 'cos', 'cos2', 'tric']
The available kernel functions#
[9]:
# Create a figure
fig = plt.figure(figsize=(12, 5))
# Enumerate every option for the kernel
for i, (ker_name, ker_class) in enumerate(kernel_switch.items()):
# Initialize the kernel object
kernel = ker_class()
# Sample from the domain
domain = kernel.domain or [-3, 3]
x_vals = np.linspace(*domain, num=2**10)
y_vals = kernel(x_vals)
# Create a subplot, set the title
ax = fig.add_subplot(3, 3, i + 1)
ax.set_title('Kernel function "{}"'.format(ker_name))
ax.plot(x_vals, y_vals, lw=3, label="{}".format(ker_name))
ax.scatter([0], [0], marker="x", color="red")
plt.grid(True, zorder=-5)
ax.set_xlim(domain)
plt.tight_layout()
The available kernel functions on three data points#
We now examine how the kernel density estimate will fit to three equally spaced data points.
[10]:
# Create three equidistant points
data = np.linspace(-1, 1, 3)
kde = sm.nonparametric.KDEUnivariate(data)
# Create a figure
fig = plt.figure(figsize=(12, 5))
# Enumerate every option for the kernel
for i, kernel in enumerate(kernel_switch.keys()):
# Create a subplot, set the title
ax = fig.add_subplot(3, 3, i + 1)
ax.set_title('Kernel function "{}"'.format(kernel))
# Fit the model (estimate densities)
kde.fit(kernel=kernel, fft=False, gridsize=2**10)
# Create the plot
ax.plot(kde.support, kde.density, lw=3, label="KDE from samples", zorder=10)
ax.scatter(data, np.zeros_like(data), marker="x", color="red")
plt.grid(True, zorder=-5)
ax.set_xlim([-3, 3])
plt.tight_layout()
A more difficult case#
The fit is not always perfect. See the example below for a harder case.
[11]:
obs_dist = mixture_rvs(
[0.25, 0.75],
size=250,
dist=[stats.norm, stats.beta],
kwargs=(dict(loc=-1, scale=0.5), dict(loc=1, scale=1, args=(1, 0.5))),
)
[12]:
kde = sm.nonparametric.KDEUnivariate(obs_dist)
kde.fit()
[12]:
<statsmodels.nonparametric.kde.KDEUnivariate at 0x7f9cc15c1450>
[13]:
fig = plt.figure(figsize=(12, 5))
ax = fig.add_subplot(111)
ax.hist(obs_dist, bins=20, density=True, edgecolor="k", zorder=4, alpha=0.5)
ax.plot(kde.support, kde.density, lw=3, zorder=7)
# Plot the samples
ax.scatter(
obs_dist,
np.abs(np.random.randn(obs_dist.size)) / 50,
marker="x",
color="red",
zorder=20,
label="Data samples",
alpha=0.5,
)
ax.grid(True, zorder=-5)
The KDE is a distribution#
Since the KDE is a distribution, we can access attributes and methods such as:
entropyevaluatecdficdfsfcumhazard
[14]:
obs_dist = mixture_rvs(
[0.25, 0.75],
size=1000,
dist=[stats.norm, stats.norm],
kwargs=(dict(loc=-1, scale=0.5), dict(loc=1, scale=0.5)),
)
kde = sm.nonparametric.KDEUnivariate(obs_dist)
kde.fit(gridsize=2**10)
[14]:
<statsmodels.nonparametric.kde.KDEUnivariate at 0x7f9cc6c92780>
[15]:
kde.entropy
[15]:
1.314324140492138
[16]:
kde.evaluate(-1)
[16]:
array([0.18085886])
Cumulative distribution, it’s inverse, and the survival function#
[17]:
fig = plt.figure(figsize=(12, 5))
ax = fig.add_subplot(111)
ax.plot(kde.support, kde.cdf, lw=3, label="CDF")
ax.plot(np.linspace(0, 1, num=kde.icdf.size), kde.icdf, lw=3, label="Inverse CDF")
ax.plot(kde.support, kde.sf, lw=3, label="Survival function")
ax.legend(loc="best")
ax.grid(True, zorder=-5)
The Cumulative Hazard Function#
[18]:
fig = plt.figure(figsize=(12, 5))
ax = fig.add_subplot(111)
ax.plot(kde.support, kde.cumhazard, lw=3, label="Cumulative Hazard Function")
ax.legend(loc="best")
ax.grid(True, zorder=-5)