Source code for gudhi.point_cloud.dtm

# This file is part of the Gudhi Library - https://gudhi.inria.fr/ - which is released under MIT.
# See file LICENSE or go to https://gudhi.inria.fr/licensing/ for full license details.
# Author(s):       Marc Glisse
#
# Copyright (C) 2020 Inria
#
# Modification(s):
#   - YYYY/MM Author: Description of the modification

from .knn import KNearestNeighbors
import numpy as np

__author__ = "Marc Glisse"
__copyright__ = "Copyright (C) 2020 Inria"
__license__ = "MIT"


[docs] class DistanceToMeasure: """ Class to compute the distance to the empirical measure defined by a point set, as introduced in :cite:`dtmgeoinference2011`. """
[docs] def __init__(self, k, q=2, **kwargs): """ Args: k (int): number of neighbors (possibly including the point itself). q (float): order used to compute the distance to measure. Defaults to 2. kwargs: same parameters as :class:`~gudhi.point_cloud.knn.KNearestNeighbors`, except that metric="neighbors" means that :func:`transform` expects an array with the distances to the k nearest neighbors. """ self.k = k self.q = q self.params = kwargs
[docs] def fit_transform(self, X, y=None): return self.fit(X).transform(X)
[docs] def fit(self, X, y=None): """ Args: X (numpy.array): coordinates for mass points. """ if self.params.setdefault("metric", "euclidean") != "neighbors": self.knn = KNearestNeighbors( self.k, return_index=False, return_distance=True, sort_results=False, **self.params ) self.knn.fit(X) return self
[docs] def transform(self, X): """ Args: X (numpy.array): coordinates for query points, or distance matrix if metric is "precomputed", or distances to the k nearest neighbors if metric is "neighbors" (if the array has more than k columns, the remaining ones are ignored). Returns: numpy.array: a 1-d array with, for each point of X, its distance to the measure defined by the argument of :func:`fit`. """ if self.params["metric"] == "neighbors": distances = X[:, : self.k] else: distances = self.knn.transform(X) distances = distances ** self.q dtm = distances.sum(-1) / self.k dtm = dtm ** (1.0 / self.q) # We compute too many powers, 1/p in knn then q in dtm, 1/q in dtm then q or some log in the caller. # Add option to skip the final root? return dtm
[docs] class DTMDensity: """ Density estimator based on the distance to the empirical measure defined by a point set, as defined in :cite:`dtmdensity`. Note that this implementation only renormalizes when asked, and the renormalization only works for a Euclidean metric, so in other cases the total measure may not be 1. .. note:: When the dimension is high, using it as an exponent can quickly lead to under- or overflows. We recommend using a small fixed value instead (for both dim and q) in those cases, even if it won't have the same nice theoretical properties as the dimension. """
[docs] def __init__(self, k=None, weights=None, q=None, dim=None, normalize=False, n_samples=None, **kwargs): """ Args: k (int): number of neighbors (possibly including the point itself). Optional if it can be guessed from weights or metric="neighbors". weights (numpy.array): weights of each of the k neighbors, optional. They are supposed to sum to 1. q (float): order used to compute the distance to measure. Defaults to dim. dim (float): final exponent representing the dimension. Defaults to the dimension, and must be specified when the dimension cannot be read from the input (metric is "neighbors" or "precomputed"). normalize (bool): normalize the density so it corresponds to a probability measure on ℝᵈ. Only available for the Euclidean metric, defaults to False. n_samples (int): number of sample points used for fitting. Only needed if `normalize` is True and metric is "neighbors". kwargs: same parameters as :class:`~gudhi.point_cloud.knn.KNearestNeighbors`, except that metric="neighbors" means that :func:`transform` expects an array with the distances to the k nearest neighbors. """ if weights is None: self.k = k if k is None: assert kwargs.get("metric") == "neighbors", 'Must specify k or weights, unless metric is "neighbors"' self.weights = None else: self.weights = np.full(k, 1.0 / k) else: self.weights = weights self.k = len(weights) assert k is None or k == self.k, "k differs from the length of weights" self.q = q self.dim = dim self.params = kwargs self.normalize = normalize self.n_samples = n_samples
[docs] def fit_transform(self, X, y=None): return self.fit(X).transform(X)
[docs] def fit(self, X, y=None): """ Args: X (numpy.array): coordinates for mass points. """ if self.params.setdefault("metric", "euclidean") != "neighbors": self.knn = KNearestNeighbors( self.k, return_index=False, return_distance=True, sort_results=False, **self.params ) self.knn.fit(X) if self.params["metric"] != "precomputed": self.n_samples = len(X) return self
[docs] def transform(self, X): """ Args: X (numpy.array): coordinates for query points, or distance matrix if metric is "precomputed", or distances to the k nearest neighbors if metric is "neighbors" (if the array has more than k columns, the remaining ones are ignored). """ q = self.q dim = self.dim if dim is None: assert self.params["metric"] not in { "neighbors", "precomputed", }, "dim not specified and cannot guess the dimension" dim = len(X[0]) if q is None: q = dim k = self.k weights = self.weights if self.params["metric"] == "neighbors": distances = np.asarray(X) if weights is None: k = distances.shape[1] weights = np.full(k, 1.0 / k) else: distances = distances[:, :k] else: distances = self.knn.transform(X) distances = distances ** q dtm = (distances * weights).sum(-1) if self.normalize: dtm /= (np.arange(1, k + 1) ** (q / dim) * weights).sum() density = dtm ** (-dim / q) if self.normalize: import math if self.params["metric"] == "precomputed": self.n_samples = len(X[0]) # Volume of d-ball Vd = math.pi ** (dim / 2) / math.gamma(dim / 2 + 1) density /= self.n_samples * Vd return density
# We compute too many powers, 1/p in knn then q in dtm, d/q in dtm then whatever in the caller. # Add option to skip the final root?