Cubix

Cubix is a simple, 100% python written, module for computing persistent homology in alternative way. Given a data cloud S of R^n, it builds a simplicial cubic complex covering S and makes a filtration over this complex using a kernel density estimator (KDE) of S. For a formal definition of the method and the simplicial cubic homology implemented, we redirect the reader to the paper 'Filtraciones en homología persistente mediante estimadores kernel de densidad' ---writen in Spanish--- available on the Github repository.

Install

You can easily install Cubix via pip:

pip install cubix

Basic usage

First of all, you must import the module:

import cubix 

The second step is choosing the data cloud to analyze. Cubix class Cloud is designed to contain these objects. You can create your cloud importing points from a CSV file just like:

X = cubix.Cloud(csv="input_file.csv")

If you have your N points of R^n stored in a numpy array (let's call it array) with shape n x N you can make a Cloud with them with:

X = cubix.Cloud(data=array)

Alternatively, Cubix has methods to generate random data clouds with some particular shapes: the spheres S⁰ (in R), S¹ (in R²) and S² (in R³) , the torus T² (in R³), the real projective spaces RP² (in R⁴), and de wedge sum of two spheres S¹vS¹ (in R²). These are subclasses of Cloud so you can easily instantiate a 2000-point cloud with S² shape like:

X = cubix.S2(center=(2,1,4), r=5, err=0.1, N=2000)

For more information about the arguments accepted to instantiate this classes, please read the documentation of each one.

Cloud class have some useful methods for plotting (when possible) and exporting data. Take a look at those 3 methods:

X.plot()
X.kde_plot()
X.export_to_csv("output.csv")

Once you have your cloud X, you can calculate the persistence homology of it. You just have to create a variable of the class PersistentHomology this way:

h = X.persistent_homology()

Of course, this will run the algorithm with default values. Arguments accepted by persistence_homology are:

• n - precision of the cubic complex covering the cloud (number of cubes per direction of R^n). Default: 10.
• margin - parameter to make the cubic complex bigger than the space occupied by the cloud. Ex: with margin=0.1 the cubic complex will take a 10% more of space. Default: 0.1
• pruning - parameter to cut off the last (the most insignificant) cubes of the filtration in order to make the algorithm faster. Ex: pruning=0.9 will keep only the 90% most significant cubes. Default: 0 (don't cut off).
• verbose - If True, print by standard error the progress of the calculation. Default: False.

Finally, you can see the results in three ways: a persistence diagram, a bar code or just explicitly printing out all born and death times:

h.persitence_diagram()
h.bar_code()
h.detail()

For more information, please check the documentation in the source code.

This software has been developed as part of the Final Degree Project in Mathematics for Universitat Autònoma de Barcelona (UAB). If you are interested in filtrations using KDE's and you understand Spanish, please take a look at the paper 'Filtraciones en homología persistente mediante estimadores kernel de densidad' available on the Github repository.