This notebook was put together by [Jake Vanderplas](http://www.vanderplas.com) for UW's [Astro 599](http://www.astro.washington.edu/users/vanderplas/Astr599/) course. Source and license info is on [GitHub](https://github.com/jakevdp/2013_fall_ASTR599/).
Scikit-learn is a collection of tools for machine learning written in Python: http://scikit-learn.org
If you're using Anaconda, simpy type
conda install scikit-learnOtherwise it's best to install from source (requires a C compiler):
git clone https://github.com/scikit-learn/scikit-learn.git
cd scikit-learn
python setup.py installScikit-learn requires NumPy and SciPy, and examples require Matplotlib.
Note: some examples below require the scripts in the fig_code directory, which
can be found within the notebooks subdirectory of the Github repository at
https://github.com/jakevdp/2013_fall_ASTR599/
Much of this material is adapted from my SciPy 2013 Tutorial, with Gael Varoquaux and Olivier Grisel
In this section we will begin to explore the basic principles of machine learning. Machine Learning is about building programs with tunable parameters (typically an array of floating point values) that are adjusted automatically so as to improve their behavior by adapting to previously seen data.
Machine Learning can be considered a subfield of Artificial Intelligence since those algorithms can be seen as building blocks to make computers learn to behave more intelligently by somehow generalizing rather that just storing and retrieving data items like a database system would do.
We'll take a look at two very simple machine learning tasks here. The first is a classification task: the figure shows a collection of two-dimensional data, colored according to two different class labels. A classification algorithm may be used to draw a dividing boundary between the two clusters of points:
In [1]:
# start the inline backend for plotting
%matplotlib inline
In [2]:
# Import the example plot from the figures directory
from fig_code import plot_sgd_separator
plot_sgd_separator()
This may seem like a trivial task, but it is a simple version of a very important concept. By drawing this separating line, we have learned a model which can generalize to new data: if you were to drop another point onto the plane which is unlabeled, this algorithm could now predict whether it's a blue or a red point.
If you'd like to see the source code used to generate this, you can either open the
code in the figures directory, or you can load the code using the %load magic command:
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#Uncomment the %load command to load the contents of the file
# %load fig_code/sgd_separator.py
The next simple task we'll look at is a regression task: a simple best-fit line to a set of data:
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from fig_code import plot_linear_regression
plot_linear_regression()
Again, this is an example of fitting a model to data, such that the model can make generalizations about new data. The model has been learned from the training data, and can be used to predict the result of test data: here, we might be given an x-value, and the model would allow us to predict the y value. Again, this might seem like a trivial problem, but it is a basic example of a type of operation that is fundamental to machine learning tasks.
Machine learning is about creating models from data: for that reason, we'll start by discussing how data can be represented in order to be understood by the computer. Along with this, we'll build on our matplotlib examples from the previous section and show some examples of how to visualize data.
Most machine learning algorithms implemented in scikit-learn expect data to be stored in a
two-dimensional array or matrix. The arrays can be
either numpy arrays, or in some cases scipy.sparse matrices.
The size of the array is expected to be [n_samples, n_features]
The number of features must be fixed in advance. However it can be very high dimensional
(e.g. millions of features) with most of them being zeros for a given sample. This is a case
where scipy.sparse matrices can be useful, in that they are
much more memory-efficient than numpy arrays.
In [4]:
from IPython.core.display import Image, display
display(Image(filename='images/iris_setosa.jpg'))
print "Iris Setosa\n"
display(Image(filename='images/iris_versicolor.jpg'))
print "Iris Versicolor\n"
display(Image(filename='images/iris_virginica.jpg'))
print "Iris Virginica"
If we want to design an algorithm to recognize iris species, what might the data be?
Remember: we need a 2D array of size [n_samples x n_features].
What would the n_samples refer to?
What might the n_features refer to?
Remember that there must be a fixed number of features for each sample, and feature
number i must be a similar kind of quantity for each sample.
Scikit-learn has a very straightforward set of data on these iris species. The data consist of the following:
Features in the Iris dataset:
Target classes to predict:
scikit-learn embeds a copy of the iris CSV file along with a helper function to load it into numpy arrays:
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from sklearn.datasets import load_iris
iris = load_iris()
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iris.keys()
Out[6]:
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n_samples, n_features = iris.data.shape
print (n_samples, n_features)
print iris.data[0]
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print iris.data.shape
print iris.target.shape
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print iris.target
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print iris.target_names
This data is four dimensional, but we can visualize two of the dimensions at a time using a simple scatter-plot:
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import numpy as np
import matplotlib.pyplot as plt
x_index = 2
y_index = 3
# this formatter will label the colorbar with the correct target names
formatter = plt.FuncFormatter(lambda i, *args: iris.target_names[int(i)])
plt.scatter(iris.data[:, x_index], iris.data[:, y_index],
c=iris.target)
plt.colorbar(ticks=[0, 1, 2], format=formatter)
plt.xlabel(iris.feature_names[x_index])
plt.ylabel(iris.feature_names[y_index]);
They come in three flavors:
sklearn.datasets.load_*sklearn.datasets.fetch_*sklearn.datasets.make_*You can explore the available dataset loaders, fetchers, and generators using IPython's
tab-completion functionality. After importing the datasets submodule from sklearn,
type
datasets.load_ + TAB
or
datasets.fetch_ + TAB
or
datasets.make_ + TAB
to see a list of available functions.
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from sklearn import datasets
In [ ]:
datasets.fetch_olivetti_faces()
Here we'll dive into the basic principles of machine learning, and how to utilize them via the Scikit-Learn API.
After briefly introducing scikit-learn's Estimator object, we'll cover supervised learning, including classification and regression problems, and unsupervised learning, including dimensinoality reduction and clustering problems.
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from sklearn.linear_model import LinearRegression
Estimator parameters: All the parameters of an estimator can be set when it is instantiated, and have suitable default values:
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model = LinearRegression(normalize=True)
print model.normalize
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print model
Estimated Model parameters: When data is fit with an estimator, parameters are estimated from the data at hand. All the estimated parameters are attributes of the estimator object ending by an underscore:
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x = np.array([0, 1, 2])
y = np.array([0, 1, 2])
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plt.plot(x, y, 'o')
plt.xlim(-0.5, 2.5)
plt.ylim(-0.5, 2.5)
Out[20]:
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# The input data for sklearn is 2D: (samples == 3 x features == 1)
X = x[:, np.newaxis]
print X
print y
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model.fit(X, y)
print model.coef_
print model.intercept_
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model.residues_
Out[24]:
The model found a line with a slope 1 and intercept 0, as we'd expect.
In Supervised Learning, we have a dataset consisting of both features and labels. The task is to construct an estimator which is able to predict the label of an object given the set of features. A relatively simple example is predicting the species of iris given a set of measurements of its flower. This is a relatively simple task. Some more complicated examples are:
What these tasks have in common is that there is one or more unknown quantities associated with the object which needs to be determined from other observed quantities.
Supervised learning is further broken down into two categories, classification and regression. In classification, the label is discrete, while in regression, the label is continuous. For example, in astronomy, the task of determining whether an object is a star, a galaxy, or a quasar is a classification problem: the label is from three distinct categories. On the other hand, we might wish to estimate the age of an object based on such observations: this would be a regression problem, because the label (age) is a continuous quantity.
In [38]:
from sklearn import neighbors, datasets
iris = datasets.load_iris()
X, y = iris.data, iris.target
# create the model
knn = neighbors.KNeighborsClassifier(n_neighbors=1)
# fit the model
knn.fit(X, y)
# What kind of iris has 3cm x 5cm sepal and 4cm x 2cm petal?
# call the "predict" method:
result = knn.predict([[3, 5, 4, 2],])
print iris.target_names[result]
In [28]:
from fig_code import plot_iris_knn
plot_iris_knn()
Exercise: Now use as an estimator on the same problem: sklearn.svm.SVC.
Note that you don't have to know what it is do use it.
If you finish early, do the same plot as above.
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from sklearn.svm import SVC
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model = SVC()
model.fit(X, y)
result = model.predict([[3, 5, 4, 2],])
print iris.target_names[result]
In [39]:
# Create some simple data
import numpy as np
np.random.seed(0)
X = np.random.random(size=(20, 1))
y = 3 * X.squeeze() + 2 + np.random.normal(size=20)
# Fit a linear regression to it
from sklearn.linear_model import LinearRegression
model = LinearRegression(fit_intercept=True)
model.fit(X, y)
print ("Model coefficient: %.5f, and intercept: %.5f"
% (model.coef_, model.intercept_))
# Plot the data and the model prediction
X_test = np.linspace(0, 1, 100)[:, np.newaxis]
y_test = model.predict(X_test)
plt.plot(X.squeeze(), y, 'o')
plt.plot(X_test.squeeze(), y_test);
Unsupervised Learning addresses a different sort of problem. Here the data has no labels, and we are interested in finding similarities between the objects in question. In a sense, you can think of unsupervised learning as a means of discovering labels from the data itself. Unsupervised learning comprises tasks such as dimensionality reduction, clustering, and density estimation. For example, in the iris data discussed above, we can used unsupervised methods to determine combinations of the measurements which best display the structure of the data. As we'll see below, such a projection of the data can be used to visualize the four-dimensional dataset in two dimensions. Some more involved unsupervised learning problems are:
Sometimes the two may even be combined: e.g. Unsupervised learning can be used to find useful features in heterogeneous data, and then these features can be used within a supervised framework.
Principle Component Analysis (PCA) is a dimension reduction technique that can find the combinations of variables that explain the most variance.
Consider the iris dataset. It cannot be visualized in a single 2D plot, as it has 4 features. We are going to extract 2 combinations of sepal and petal dimensions to visualize it:
In [40]:
X, y = iris.data, iris.target
from sklearn.decomposition import PCA
pca = PCA(n_components=2)
pca.fit(X)
X_reduced = pca.transform(X)
print "Reduced dataset shape:", X_reduced.shape
import pylab as pl
pl.scatter(X_reduced[:, 0], X_reduced[:, 1], c=y)
print "Meaning of the 2 components:"
for component in pca.components_:
print " + ".join("%.3f x %s" % (value, name)
for value, name in zip(component,
iris.feature_names))
In [41]:
from sklearn.cluster import KMeans
k_means = KMeans(n_clusters=3, random_state=0) # Fixing the RNG in kmeans
k_means.fit(X)
y_pred = k_means.predict(X)
pl.scatter(X_reduced[:, 0], X_reduced[:, 1], c=y_pred);
Scikit-learn strives to have a uniform interface across all methods,
and we'll see examples of these below. Given a scikit-learn estimator
object named model, the following methods are available:
model.fit() : fit training data. For supervised learning applications,
this accepts two arguments: the data X and the labels y (e.g. model.fit(X, y)).
For unsupervised learning applications, this accepts only a single argument,
the data X (e.g. model.fit(X)).model.predict() : given a trained model, predict the label of a new set of data.
This method accepts one argument, the new data X_new (e.g. model.predict(X_new)),
and returns the learned label for each object in the array.model.predict_proba() : For classification problems, some estimators also provide
this method, which returns the probability that a new observation has each categorical label.
In this case, the label with the highest probability is returned by model.predict().model.score() : for classification or regression problems, most (all?) estimators implement
a score method. Scores are between 0 and 1, with a larger score indicating a better fit.model.transform() : given an unsupervised model, transform new data into the new basis.
This also accepts one argument X_new, and returns the new representation of the data based
on the unsupervised model.model.fit_transform() : some estimators implement this method,
which more efficiently performs a fit and a transform on the same input data.Here we'll show a couple examples of machine learning on astronomical data. For many more examples, see the AstroML website.
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from astroML.datasets import fetch_rrlyrae_combined
from sklearn.cross_validation import train_test_split
X, y = fetch_rrlyrae_combined()
# For now, we'll only fit the first two colors
X_train, X_test, y_train, y_test = train_test_split(X, y)
In [43]:
N_plot = 5000
plt.scatter(X[-N_plot:, 0], X[-N_plot:, 1], c=y[-N_plot:],
edgecolors='none')
plt.xlabel('u-g color')
plt.ylabel('g-r color');
Red points are RR-Lyrae, Blue points are main sequence stars.
Now we'll do a simple and fast $K$-neighbors classification.
Note that we train on part of the data and test on another part. Otherwise, an estimator which simply remembers the entire dataset would obtain a perfect classification!
In [44]:
from sklearn.neighbors import KNeighborsClassifier
clf = KNeighborsClassifier(n_neighbors=5)
clf.fit(X_train, y_train)
y_pred = clf.predict(X_test)
In [45]:
print np.sum(y_pred == y_test)
print np.sum(y_pred != y_test)
In [46]:
from sklearn.metrics import classification_report
print classification_report(y_test, y_pred,
target_names=['MS star', 'RR Lyrae'])
The range for precision, recall, and F1 score is 0 to 1, with 1 being perfect. Often in astronomy, we call the recall the completeness, and (1 - precision) the contamination.
Because this is an unbalanced dataset, we see that the RR Lyrae stars are completely overwhelmed by the larger number of normal Main Sequence stars.
Use another classifier and try to improve on this precision/recall score.
There are several you might try:
sklearn.neighbors.GaussianNaiveBayes (slow but inaccurate)sklearn.lda.LDA (slow but inaccurate)sklearn.svm.SVC (fast but accurate)sklearn.svm.SVC with kernel='rbf' (fast but accurate)sklearn.ensemble.RandomForestClassifier (fast & potentially accurate with tuning)For the slower algorithms, it might be a good idea to use only part of the dataset as you experiment, i.e. when training do something like the following:
clf.fit(X_train[::5], y_train[::5])Once you're happy, you can run the training on the full dataset.
What's the best precision/recall you can obtain for the RR-Lyrae data?
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from astroML.datasets import fetch_sdss_specgals
In [48]:
data = fetch_sdss_specgals()
# put magnitudes in a matrix
X = np.vstack([data['modelMag_%s' % f] for f in 'ugriz']).T
y = data['z']
# Split into training and testing data
X_train, X_test, y_train, y_test = train_test_split(X, y)
In [49]:
from sklearn.linear_model import LinearRegression
est = LinearRegression()
est.fit(X_train, y_train)
y_pred = est.predict(X_test)
In [50]:
plt.plot(y_test, y_pred, ',k')
plt.plot([0, 1], [0, 1], ':k')
plt.xlim(0, 0.6)
plt.ylim(0, 0.6)
Out[50]:
Evidently, a simple linear model is not a very good fit!
Let's compute the RMS deviation to see how poor this actually is:
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rms = np.sqrt(np.mean((y_test - y_pred) ** 2))
print rms
Try to improve on this result using another regression algorithm. Some potential choices:
sklearn.neighbors.KNeighborsRegressor (fast-ish, but often inaccuratesklearn.svm.SVR (potentially accurate, but slow)sklearn.ensemble.RandomForestRegressor (fast, and accurate with tuning)sklearn.ensemble.GradientBoostingRegressor (accurate with tuning, can be very slow depending on parameters)Again, sub-sampling the data can help as you explore some of the slower techniques.
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from sklearn.ensemble import RandomForestClassifier
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RandomForestClassifier?
There's lots more information out there.
A couple of resources I've worked on: