genieclust.Genie¶

class
genieclust.
Genie
(n_clusters=2, *, gini_threshold=0.3, M=1, affinity='l2', exact=True, compute_full_tree=False, compute_all_cuts=False, postprocess='boundary', cast_float32=True, mlpack_enabled='auto', mlpack_leaf_size=1, nmslib_n_neighbors=64, nmslib_params_init={'method': 'hnsw'}, nmslib_params_index={'post': 2}, nmslib_params_query={}, verbose=False)¶ Genie++ hierarchical clustering algorithm
 Parameters
 n_clustersint
Number of clusters to detect.
If M > 1 and postprocess is not
"all"
, n_clusters = 1 can act as a noise point/outlier detector. The approximate method (see parameter exact) can sometimes fail to detect the coarsestgrained partitions; in such a case, more clusters might be returned (with a warning). gini_thresholdfloat
Threshold for the Genie correction in [0,1].
The Gini index is used to quantify the inequality of the cluster size distribution. Low thresholds highly penalise the formation of small clusters. Threshold of 1.0 disables the correction and for M = 1 makes the method be equivalent to the single linkage algorithm.
The algorithm tends to be stable with respect to small changes to the threshold — they do not tend to affect the output clustering. Usually, thresholds of 0.1, 0.3, 0.5, and 0.7 are worth giving a try.
 Mint
Smoothing factor for the mutual reachability distance [6].
M = 1 gives the original Genie algorithm [1] (with no noise point detection) with respect to the chosen affinity asis. Note that for M > 1 we need additionally \(O(M n)\) working memory for storing of points’ nearest neighbours.
 affinitystr
Metric used to compute the linkage.
For exact =
True
:One of:
"l2"
(synonym:"euclidean"
),"l1"
(synonym:"manhattan"
,"cityblock"
),"cosinesimil"
(synonym:"cosine"
), or"precomputed"
.In the latter case, the X argument to the fit method must be a distance vector or a squareform distance matrix, see scipy.spatial.distance.pdist.
For exact =
False
:Any dissimilarity supported by nmslib, see [5] and https://github.com/nmslib/nmslib/blob/master/manual/spaces.md, for instance:
"l2"
,"l2_sparse"
,"l1"
,"l1_sparse"
,"linf"
,"linf_sparse"
,"cosinesimil"
,"cosinesimil_sparse"
,"negdotprod"
,"negdotprod_sparse"
,"angulardist"
,"angulardist_sparse"
,"leven"
,"normleven"
,"jaccard_sparse"
,"bit_jaccard"
,"bit_hamming"
.
 exactbool
Whether to compute the minimum spanning tree exactly or rather estimate it based on an approximate nearneighbour graph.
The exact method has time complexity of \(O(d n^2)\) [2] (however, see mlpack_enabled) but only needs \(O(n)\) memory.
If exact is
False
, the minimum spanning tree is approximated based on an approximate \(k\)nearest neighbours graph found by nmslib [5]. This is typically very fast but requires \(O(k n)\) memory. compute_full_treebool
Whether to determine the whole cluster hierarchy and the linkage matrix.
Only available if M = 1 and exact is
True
. Enables plotting of dendrograms or cutting of the hierarchy at an arbitrary level, see the children_, distances_, counts_ attributes. compute_all_cutsbool
Whether to compute the requested n_clusterspartition and all the coarsergrained ones.
If
True
, then the labels_ attribute will be a matrix, see below. postprocess{“boundary”, “none”, “all”}
Controls the treatment of noise points after the clusters are identified.
In effect only if M > 1. Each leaf in the minimum spanning tree is treated as a noise point. We call it a boundary point if it is amongst its adjacent vertex’s M  1 nearest neighbours. By default, only boundary points are merged with their nearest core points.
To force a classical n_clusterspartition of a data set (with no notion of noise), choose
"all"
. Furthermore,"none"
leaves all leaves, i.e., noise points (including the boundary ones) asis. cast_float32bool
Whether casting of data type to
float32
is to be performed.If exact is
True
, it decreases the runtime ca. 2 times at a cost of greater memory use. Otherwise, note that nmslib requiresfloat32
data anyway when using dense or sparse numeric matrix inputs.By setting cast_float32 to
False
a user assures themself that the inputs are of acceptable form. mlpack_enabled“auto” or bool
Whether mlpack.emst should be used for computing the Euclidean minimum spanning tree instead of the JarníkPrim algorithm when exact is
True
.Often fast for very lowdimensional spaces. As the name suggests, only affinity of
'l2'
is supported (and M = 1). By default, we rely on mlpack if it is installed and n_features <= 6. mlpack_leaf_sizeint
Leaf size in the kdtree when mlpack.emst is used.
According to the mlpack manual, leaves of size 1 give the best performance at the cost of greater memory use.
 nmslib_n_neighborsint
The number of approximate nearest neighbours used to estimate the minimum spanning tree when when exact is
False
.If the number of nearest neighbours is too small, the nearest neighbour graph might be disconnected and the number of obtained clusters might be greater than the requested one.
nmslib_n_neighbors must not be less than M  1.
 nmslib_params_initdict
A dictionary of parameters to be passed to nmslib.init when exact is
False
.See https://github.com/nmslib/nmslib/blob/master/manual/methods.md, https://github.com/nmslib/nmslib/blob/master/manual/spaces.md and https://nmslib.github.io/nmslib/ for more details. The space, data_type, and dtype parameters will be set based on the chosen affinity and the input X.
 nmslib_params_indexdict
A dictionary of parameters to be passed to index.createIndex, where index is the object constructed with nmslib.init.
The indexThreadQty parameter will be set based on the
OMP_NUM_THREADS
environment variable. nmslib_params_querydict
A dictionary of parameters to be passed to index.setQueryTimeParams, where index is the object constructed with nmslib.init.
 verbosebool
Whether to print diagnostic messages and progress information on
stderr
.
Notes
Genie is a robust and outlier resistant hierarchical clustering algorithm [1], originally published as an R package
genie
. This new implementation is, amongst others, much faster and now features optional smoothing and noise point detection (if M > 1).Genie is based on a minimum spanning tree (MST) of the pairwise distance graph of a given point set. Just like the single linkage, it consumes the edges of the MST in increasing order of weights. However, it prevents the formation of clusters of highly imbalanced sizes; once the Gini index of the cluster size distribution raises above an assumed threshold, a forced merge of a point group of the smallest size is performed. Its appealing simplicity goes hand in hand with its usability; Genie often outperforms other clustering approaches on benchmark data.
The Genie algorithm itself has \(O(n \sqrt{n})\) time and \(O(n)\) memory complexity provided that a minimum spanning tree of the pairwise distance graph is given. Generally, our parallelised implementation of a Jarník (Prim/Dijkstra)like method [2] will be called to compute an MST, which takes \(O(d n^2)\) time. However, mlpack [3] provides a very fast alternative in the case of Euclidean spaces of (very) low dimensionality and M = 1, see [4] and the mlpack_enabled parameter. Moreover, in the approximate method (exact =
False
) we apply the Kruskal algorithm on the nearneighbour graph determined by nmslib [5]. Albeit this only gives some sort of a spanning forest, such a data structure turns out to be very suitable for our clustering task (note that the set of connected components will determine the top level of the identified cluster hierarchy).The Genie correction together with the smoothing factor M > 1 gives a robustified version of the HDBSCAN* [6] algorithm that, contrary to its predecessor, is able to detect a predefined number of clusters. Hence, it is independent of the DBSCAN’s somewhat magical
eps
parameter or the HDBSCAN’smin_cluster_size
one. If M > 1, then the minimum spanning tree is computed with respect to the mutual reachability distance (based, e.g., on the Euclidean metric). Formally, the distance \(m(i,j)\) is used instead of the chosen “raw” distance, \(d(i,j)\). It holds \(m(i,j)=\max(d(i,j), c(i), c(j))\), where the “core” distance \(c(i)\) is given by \(d(i,k)\) with \(k\) being the (M  1)th nearest neighbour of \(i\). This makes “noise” and “boundary” points being “pulled away” from each other, however, note that M = 2 corresponds to the original distance. During the clustering procedure, all leaves of the MST do not take part in the clustering process. They may be merged with the nearest clusters during the postprocessing stage, or left marked as “noise” observations. Environment variables
 OMP_NUM_THREADS
Controls the number of threads used for computing the minimum spanning tree (not supported by mlpack).
References
 1(1,2)
Gagolewski M., Bartoszuk M., Cena A., Genie: A new, fast, and outlierresistant hierarchical clustering algorithm, Information Sciences 363, 2016, 823. doi:10.1016/j.ins.2016.05.003.
 2(1,2)
Olson C.F., Parallel algorithms for hierarchical clustering, Parallel Computing 21(8), 1995, 13131325. doi:10.1016/01678191(95)00017I.
 3
Curtin R.R., Edel M., Lozhnikov M., Mentekidis Y., Ghaisas S., Zhang S., mlpack 3: A fast, flexible machine learning library, Journal of Open Source Software 3(26), 726, 2018. doi:10.21105/joss.00726.
 4
March W.B., Ram P., Gray A.G., Fast Euclidean Minimum Spanning Tree: Algorithm, Analysis, and Applications, Proc. ACM SIGKDD’10, 2010, 603611.
 5(1,2,3)
Naidan B., Boytsov L., Malkov Y., Novak D., Nonmetric space library (NMSLIB) manual, version 2.0, 2019. https://github.com/nmslib/nmslib/blob/master/manual/latex/manual.pdf.
 6(1,2)
Campello R., Moulavi D., Zimek A., Sander J., Hierarchical density estimates for data clustering, visualization, and outlier detection, ACM Transactions on Knowledge Discovery from Data 10(1), 2015, 5:1–5:51. doi:10.1145/2733381.
 Attributes
 labels_ndarray
Detected cluster labels.
If compute_all_cuts is
False
(the default), this is an integer vector such thatlabels_[i]
gives the cluster ID (between 0 and n_clusters_  1) of the ith object. If M > 1, noise points are labelled 1 (unless taken care of in the postprocessing stage).Otherwise, i.e., if compute_all_cuts is
True
, all partitions of cardinality down to n_clusters are determined;labels_[j,i]
denotes the cluster ID of the ith point in a jpartition. We assume that both the 0 and 1 partition distinguishes only between noise and nonnoise points, however, no postprocessing is conducted on the 0partition (there might be points with labels of 1 even if postprocess is"all"
).Note that the approximate method (exact of
False
) might fail to determine the finegrained clusters (if the approximate neighbour graph is disconnected)  the actual number of clusters detected can be larger. n_clusters_int
The actual number of clusters detected by the algorithm.
As we argued above, the approximate method might sometimes yield a more finegrained partition than the requested one (with a warning). Moreover, there might be too many noise points in the dataset.
 n_samples_int
The number of points in the fitted dataset.
 n_features_int
The number of features in the fitted dataset.
If the information is not available, it is be set to 1.
 children_None or ndarray
If compute_full_tree is
True
, this is a matrix whose ith row provides the information on the clusters merged in the ith iteration. See the description ofZ[:,0]
andZ[:,1]
in scipy.cluster.hierarchy.linkage. Together with distances_ and counts_, this constitutes the linkage matrix that can be used for plotting the dendrogram. distances_None or ndarray
If compute_full_tree is
True
, this is a vector that gives the distance between two clusters merged in each iteration, see the description ofZ[:,2]
in scipy.cluster.hierarchy.linkage.As the original Genie algorithm does not guarantee that that distances are ordered increasingly (there are other hierarchical clustering linkages that violate the ultrametricity property as well), these are corrected by applying
distances_ = genieclust.tools.cummin(distances_[::1])[::1]
. counts_None or ndarray
If compute_full_tree is
True
, this is a vector giving the number of elements in a cluster created in each iteration. See the description ofZ[:,3]
in scipy.cluster.hierarchy.linkage.
Methods
fit
(X[, y])Perform cluster analysis of a dataset.
fit_predict
(X[, y])Perform cluster analysis of a dataset and return the predicted labels.
get_params
([deep])Get parameters for this estimator.
set_params
(**params)Set the parameters of this estimator.

fit
(X, y=None)¶ Perform cluster analysis of a dataset.
 Parameters
 Xobject
Typically a matrix with
n_samples
rows andn_features
columns, see below for more details and options. yNone
Ignored.
 Returns
 selfgenieclust.Genie
The object that the method was called on.
Notes
Refer to the labels_ and n_clusters_ attributes for the result.
Acceptable X types depend whether we use the exact or the approximate method.
X when exact =
True
.For affinity of
"precomputed"
, X should either be a distance vector of lengthn_samples*(n_samples1)/2
(see scipy.spatial.distance.pdist) or a square distance matrix of shape(n_samples, n_samples)
(see scipy.spatial.distance.squareform).Otherwise, X should be realvalued matrix (dense
numpy.ndarray
, or an object coercible to) withn_samples
rows andn_features
columns.In the latter case, it might be a good idea to standardise or at least somehow preprocess the coordinates of the input data points by calling, for instance,
X = (XX.mean(axis=0))/X.std(axis=None, ddof=1)
so that the dataset is centred at 0 and has total variance of 1. This way the method becomes translation and scale invariant. What’s more, if data are recorded with small precision (say, up to few decimal digits), adding a tiny bit of Gaussian noise will assure the solution is unique (note that this generally applies to other distancebased clustering algorithms as well).X when exact =
False
.The approximate method relies on nmslib for locating the nearest neighbours. Therefore, it supports all datatypes described in https://github.com/nmslib/nmslib/blob/master/manual/spaces.md. Depending on the chosen affinity, X may hence be a realvalued
numpy.ndarray
matrix withn_samples
rows andn_features
columns, ascipy.sparse.csr_matrix
object, or an array of ASCII strings.
References
 1
Naidan B., Boytsov L., Malkov Y., Novak D., Nonmetric space library (NMSLIB) manual, version 2.0, 2019. https://github.com/nmslib/nmslib/blob/master/manual/latex/manual.pdf.