Programming Exercise 8: Anomaly Detection and Recommender Systems Solution

Introduction

In this exercise, you will implement the anomaly detection algorithm and apply it to detect failing servers on a network. In the second part, you will use collaborative ltering to build a recommender system for movies. Before starting on the programming exercise, we strongly recommend watching the video lectures and completing the review questions for the associated topics.

To get started with the exercise, you will need to download the starter code and unzip its contents to the directory where you wish to complete the exercise. If needed, use the cd command in Octave to change to this directory before starting this exercise.

Files included in this exercise

ex8.m - Octave/Matlab script for    rst part of exercise

ex8 cofi.m - Octave/Matlab script for second part of exercise ex8data1.mat - First example Dataset for anomaly detection ex8data2.mat - Second example Dataset for anomaly detection ex8 movies.mat - Movie Review Dataset


ex8 movieParams.mat - Parameters provided for debugging multivariateGaussian.m - Computes the probability density function for a Gaussian distribution


visualizeFit.m - 2D plot of a Gaussian distribution and a dataset checkCostFunction.m - Gradient checking for collaborative ltering computeNumericalGradient.m - Numerically compute gradients fmincg.m - Function minimization routine (similar to fminunc) loadMovieList.m - Loads the list of movies into a cell-array


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movie ids.txt - List of movies

normalizeRatings.m - Mean normalization for collaborative    ltering

[?] estimateGaussian.m - Estimate the parameters of a Gaussian dis-tribution with a diagonal covariance matrix

[?] selectThreshold.m - Find a threshold for anomaly detection

[?] cofiCostFunc.m - Implement the cost function for collaborative l-tering


    • indicates  les you will need to complete

Throughout the rst part of the exercise (anomaly detection) you will be using the script ex8.m. For the second part of collaborative ltering, you will use ex8 cofi.m. These scripts set up the dataset for the problems and make calls to functions that you will write. You are only required to modify functions in other les, by following the instructions in this assignment.


Where to get help

We also strongly encourage using the online Q&A Forum to discuss exer-cises with other students. However, do not look at any source code written by others or share your source code with others.

If you run into network errors using the submit script, you can also use an online form for submitting your solutions. To use this alternative submis-sion interface, run the submitWeb script to generate a submission le (e.g., submit ex8 part2.txt). You can then submit this le through the web submission form in the programming exercises page (go to the programming exercises page, then select the exercise you are submitting for). If you are having no problems submitting through the standard submission system us-ing the submit script, you do not need to use this alternative submission interface.





    • Anomaly detection

In this exercise, you will implement an anomaly detection algorithm to detect anomalous behavior in server computers. The features measure the through-put (mb/s) and latency (ms) of response of each server. While your servers were operating, you collected m = 307 examples of how they were behaving,


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and thus have an unlabeled dataset fx(1); : : : ; x(m)g. You suspect that the vast majority of these examples are \normal" (non-anomalous) examples of the servers operating normally, but there might also be some examples of servers acting anomalously within this dataset.

You will use a Gaussian model to detect anomalous examples in your dataset. You will rst start on a 2D dataset that will allow you to visualize what the algorithm is doing. On that dataset you will t a Gaussian dis-tribution and then nd values that have very low probability and hence can be considered anomalies. After that, you will apply the anomaly detection algorithm to a larger dataset with many dimensions. You will be using ex8.m for this part of the exercise.

The    rst part of ex8.m will visualize the dataset as shown in Figure 1.








Throughput (mb/s)

30



25


20


15


10


5


0
0    5    10    15    20    25    30

Latency (ms)

Figure 1: The    rst dataset.



1.1    Gaussian distribution

To perform anomaly detection, you will rst need to t a model to the data’s distribution.

Given a training set fx(1); :::; x(m)g (where x(i) 2 Rn), you want to esti-mate the Gaussian distribution for each of the features xi. For each feature i = 1 : : : n, you need to nd parameters i and i2 that t the data in the i-th dimension fx(1)i; :::; x(im)g (the i-th dimension of each example).


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The Gaussian distribution is given by

1
(x   )2
p(x;  ;  2) =
p





e

;




2 2



2  2





where    is the mean and    2 controls the variance.

1.2    Estimating parameters for a Gaussian

You can estimate the parameters, ( i, i2), of the i-th feature by using the following equations. To estimate the mean, you will use:


i =

1

m
xi(j)
;
(1)



m
=1













and for the variance you will use:



Xj











2 =
1


m
(x(j)
i)2:
(2)



Xj



i
m

i














=1














Your task is to complete the code in estimateGaussian.m. This function takes as input the data matrix X and should output an n-dimension vector mu that holds the mean of all the n features and another n-dimension vector sigma2 that holds the variances of all the features. You can implement this using a for-loop over every feature and every training example (though a vec-torized implementation might be more e cient; feel free to use a vectorized implementation if you prefer). Note that in Octave, the var function will (by default) use m1 1 , instead of m1 , when computing i2.

Once you have completed the code in estimateGaussian.m, the next part of ex8.m will visualize the contours of the tted Gaussian distribution. You should get a plot similar to Figure 2. From your plot, you can see that most of the examples are in the region with the highest probability, while the anomalous examples are in the regions with lower probabilities.

You should now submit your estimate Gaussian parameters function.

1.3    Selecting the threshold, "

Now that you have estimated the Gaussian parameters, you can investigate which examples have a very high probability given this distribution and which examples have a very low probability. The low probability examples are

4






30







25







20






(mb/s)







Throughput
15















10







5







0
5
10
15
20
25
30

0







Latency (ms)

Figure 2: The Gaussian distribution contours of the distribution t to the dataset.

more likely to be the anomalies in our dataset. One way to determine which examples are anomalies is to select a threshold based on a cross validation set. In this part of the exercise, you will implement an algorithm to select the threshold " using the F1 score on a cross validation set.

You should now complete the code in selectThreshold.m. For this, we will use a cross validation set f(x(1)cv; ycv(1)); : : : ; (x(cvmcv); ycv(mcv))g, where the la-bel y = 1 corresponds to an anomalous example, and y = 0 corresponds

to a normal
example.  For each cross validation example,
we will
com-
(i)
(1)

(mcv)
) is
pute p(xcv ).
The vector of all of these probabilities p(xcv
); : : : ; p(xcv


passed to selectThreshold.m in the vector pval. The corresponding labels ycv(1); : : : ; ycv(mcv) is passed to the same function in the vector yval.

The function selectThreshold.m should return two values; the rst is the selected threshold ". If an example x has a low probability p(x) < ", then it is considered to be an anomaly. The function should also return the F1 score, which tells you how well you’re doing on nding the ground truth anomalies given a certain threshold. For many di erent values of ", you will compute the resulting F1 score by computing how many examples the current threshold classi es correctly and incorrectly.
The F1 score is computed using precision (prec) and recall (rec):

F1 =
2  prec  rec
;
(3)

prec + rec








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You compute precision and recall by:

prec
=
tp

(4)









tp + f p


rec
=
tp
;
(5)








tp + f n



where

    • tp is the number of true positives: the ground truth label says it’s an anomaly and our algorithm correctly classi ed it as an anomaly.

    • f p is the number of false positives: the ground truth label says it’s not an anomaly, but our algorithm incorrectly classi ed it as an anomaly.

    • f n is the number of false negatives: the ground truth label says it’s an anomaly, but our algorithm incorrectly classi ed it as not being anoma-lous.

In the provided code selectThreshold.m, there is already a loop that will try many di erent values of " and select the best " based on the F1 score.

You should now complete the code in selectThreshold.m. You can im-plement the computation of the F1 score using a for-loop over all the cross validation examples (to compute the values tp, f p, f n). You should see a value for epsilon of about 8.99e-05.


Implementation Note: In order to compute tp, f p and f n, you may be able to use a vectorized implementation rather than loop over all the examples. This can be implemented by Octave’s equality test between a vector and a single number. If you have several binary values in an n-dimensional binary vector v 2 f0; 1gn, you can nd out how many values in this vector are 0 by using: sum(v == 0). You can also apply a logical and operator to such binary vectors. For instance, let cvPredictions be a binary vector of the size of your number of cross validation set, where the i-th element is 1 if your algorithm considers x(cvi) an anomaly, and 0 otherwise. You can then, for example, compute the number of false positives using: fp = sum((cvPredictions == 1) & (yval == 0)).


Once you have completed the code in selectThreshold.m, the next step in ex8.m will run your anomaly detection code and circle the anomalies in the plot (Figure 3).

You should now submit your select threshold function.

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30







25







20






(mb/s)







Throughput
15















10







5







0
5
10
15
20
25
30

0







Latency (ms)

Figure 3: The classi ed anomalies.

1.4    High dimensional dataset

The last part of the script ex8.m will run the anomaly detection algorithm you implemented on a more realistic and much harder dataset. In this dataset, each example is described by 11 features, capturing many more properties of your compute servers.

The script will use your code to estimate the Gaussian parameters ( i and i2), evaluate the probabilities for both the training data X from which you estimated the Gaussian parameters, and do so for the the cross-validation set Xval. Finally, it will use selectThreshold to nd the best threshold ". You should see a value epsilon of about 1.38e-18, and 117 anomalies found.





    • Recommender Systems

In this part of the exercise, you will implement the collaborative ltering learning algorithm and apply it to a dataset of movie ratings.1 This dataset consists of ratings on a scale of 1 to 5. The dataset has nu = 943 users, and nm = 1682 movies. For this part of the exercise, you will be working with the script ex8 cofi.m.


1MovieLens 100k Dataset from GroupLens Research.

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In the next parts of this exercise, you will implement the function cofiCostFunc.m that computes the collaborative tlering objective function and gradient. Af-

ter implementing the cost function and gradient, you will use fmincg.m to learn the parameters for collaborative ltering.

2.1    Movie ratings dataset

The rst part of the script ex8 cofi.m will load the dataset ex8 movies.mat, providing the variables Y and R in your Octave environment.


The matrix Y (a num movies num users matrix) stores the ratings y(i;j) (from 1 to 5). The matrix R is an binary-valued indicator matrix, where R(i; j) = 1 if user j gave a rating to movie i, and R(i; j) = 0 otherwise. The objective of collaborative ltering is to predict movie ratings for the movies that users have not yet rated, that is, the entries with R(i; j) = 0. This will allow us to recommend the movies with the highest predicted ratings to the user.


To help you understand the matrix Y, the script ex8 cofi.m will compute the average movie rating for the rst movie (Toy Story) and output the average rating to the screen.


Throughout this part of the exercise, you will also be working with the matrices, X and Theta:

2
| (x(2))T |
3


2
| ( (2))T |
3


6
| (x(1))T |
7


6
| ( (1))T |
7

X =

...

;
Theta =

...

:

6
| (x(nm))T |
7


6
| ( (nu))T |
7


6

7


6

7


4

5


4

5

The i-th row of X corresponds to the feature vector x(i) for the i-th movie, and the j-th row of Theta corresponds to one parameter vector (j), for the j-th user. Both x(i) and (j) are n-dimensional vectors. For the purposes of this exercise, you will use n = 100, and therefore, x(i) 2 R100 and (j) 2 R100. Correspondingly, X is a nm 100 matrix and Theta is a nu 100 matrix.

2.2    Collaborative    ltering learning algorithm

Now, you will start implementing the collaborative ltering learning algo-rithm. You will start by implementing the cost function (without regulariza-tion).

The collaborative ltering algorithm in the setting of movie recommen-dations considers a set of n-dimensional parameter vectors x(1); :::; x(nm) and

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(1); :::; (nu), where the model predicts the rating for movie i by user j as y(i;j) = ( (j))T x(i). Given a dataset that consists of a set of ratings produced by some users on some movies, you wish to learn the parameter vectors x(1); :::; x(nm); (1); :::; (nu) that produce the best t (minimizes the squared error).

You will complete the code in cofiCostFunc.m to compute the cost func-tion and gradient for collaborative ltering. Note that the parameters to the function (i.e., the values that you are trying to learn) are X and Theta. In order to use an o -the-shelf minimizer such as fmincg, the cost function has been set up to unroll the parameters into a single vector params. You had previously used the same vector unrolling method in the neural networks programming exercise.

2.2.1    Collaborative    ltering cost function

The collaborative    ltering cost function (without regularization) is given by


1
(i;j):Xr(
J(x(1); :::; x(nm); (1); :::; (nu)) =

(( (j))T x(i)    y(i;j))2:

2

i;j)=1

You should now modify cofiCostFunc.m to return this cost in the vari-able J. Note that you should be accumulating the cost for user j and movie

    • only if R(i; j) = 1.

After you have completed the function, the script ex8 cofi.m will run your cost function. You should expect to see an output of 22:22.


You should now submit your cost function.




















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Implementation Note: We strongly encourage you to use a vectorized implementation to compute J, since it will later by called many times by the optimization package fmincg. As usual, it might be easiest to rst write a non-vectorized implementation (to make sure you have the right answer), and the modify it to become a vectorized implementation (checking that the vectorization steps don’t change your algorithm’s out-put). To come up with a vectorized implementation, the following tip might be helpful: You can use the R matrix to set selected entries to 0. For example, R .* M will do an element-wise multiplication between M and R; since R only has elements with values either 0 or 1, this has the e ect of setting the elements of M to 0 only when the corresponding value in R is 0. Hence, sum(sum(R.*M)) is the sum of all the elements of M for which the corresponding element in R equals 1.


2.2.2    Collaborative    ltering gradient

Now, you should implement the gradient (without regularization). Speci - cally, you should complete the code in cofiCostFunc.m to return the vari-ables X grad and Theta grad. Note that X grad should be a matrix of the same size as X and similarly, Theta grad is a matrix of the same size as Theta. The gradients of the cost function is given by:



@J
=
(( (j))T x(i)
y(i;j)) k(j)







@x(i)

j:rX(




i;j)=1


k




@J
=
(( (j))T x(i)
y(i;j))x(i):






@ (j)

X(
k






i:r i;j)=1


k




Note that the function returns the gradient for both sets of variables by unrolling them into a single vector. After you have completed the code to compute the gradients, the script ex8 cofi.m will run a gradient check (checkCostFunction) to numerically check the implementation of your gra-dients.2 If your implementation is correct, you should nd that the analytical and numerical gradients match up closely.


You should now submit your collaborative    ltering gradient function.


    • This is similar to the numerical check that you used in the neural networks exercise.





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Implementation Note: You can get full credit for this assignment without using a vectorized implementation, but your code will run much more slowly (a small number of hours), and so we recommend that you try to vectorize your implementation.

To get started, you can implement the gradient with a for-loop over movies

(for computing @J(i) ) and a for-loop over users (for computing    ). When

@xk
you rst implement the gradient, you might start with an unvectorized version, by implementing another inner for-loop that computes each ele-ment in the summation. After you have completed the gradient computa-tion this way, you should try to vectorize your implementation (vectorize the inner for-loops), so that you’re left with only two for-loops (one for

looping over movies to compute    for each movie, and one for looping


over users to compute  @J(j)  for each user).

@ k






































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Implementation Tip: To perform the vectorization, you might  nd this

helpful: You should come up with a way to compute all the derivatives
associated with x(1i); x(2i); : : : ; x(ni) (i.e., the derivative terms associated with the feature vector x(i)) at the same time. Let us de ne the derivatives for the feature vector of the i-th movie as:
2@J3

@x(1i)
6@J7

6 (i) 7
(Xgrad(i; :))T = 6@x.2 7 = 6..7
4    5
@J

@x(ni)


X
(( (j))T x(i)    y(i;j)) (j)

j:r(i;j)=1

To vectorize the above expression, you can start by indexing into Theta and Y to select only the elements of interests (that is, those with r(i; j) = 1). Intuitively, when you consider the features for the i-th movie, you only need to be concern about the users who had given ratings to the movie, and this allows you to remove all the other users from Theta and Y.

Concretely, you can set idx = find(R(i, :)==1) to be a list of all the users that have rated movie i. This will allow you to create the temporary matrices Thetatemp = Theta(idx; :) and Ytemp = Y(i; idx) that index into Theta and Y to give you only the set of users which have rated the i-th movie. This will allow you to write the derivatives as:

Xgrad(i; :) = (X(i; :)    ThetaTtemp    Ytemp)    Thetatemp:

(Note: The vectorized computation above returns a row-vector instead.)

After you have vectorized the computations of the derivatives with respect to x(i), you should use a similar method to vectorize the derivatives with respect to (j) as well.


2.2.3    Regularized cost function

The cost function for collaborative    ltering with regularization is given by











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1






J(x(1); :::; x(nm); (1); :::; (nu)) =

(i;j):Xr(
(( (j))T x(i)

2




2
i;j)=1
( k ))2
!
+


nu
n







(j






XXk















j=1
=1











y(i;j))2+

2

(xk(i))2!
:

nm
n


XXk





i=1
=1


You should now add regularization to your original computations of the cost function, J. After you are done, the script ex8 cofi.m will run your regularized cost function, and you should expect to see a cost of about 31.34.


You should now submit your regularized cost function.

2.2.4    Regularized gradient

Now that you have implemented the regularized cost function, you should proceed to implement regularization for the gradient. You should add to your implementation in cofiCostFunc.m to return the regularized gradient by adding the contributions from the regularization terms. Note that the gradients for the regularized cost function is given by:


@J
=
(( (j))T x(i)
y(i;j)) (j) +  x(i)






@x(i)
j:rX(
k
k







i;j)=1



k





@J
=
(( (j))T x(i)
y(i;j))x(i) +   (j):






@ (j)
i:r
X(
k
k







i;j)=1



k





This means that you just need to add x(i) to the X grad(i,:) variable described earlier, and add (j) to the Theta grad(j,:) variable described earlier.


After you have completed the code to compute the gradients, the script ex8 cofi.m will run another gradient check (checkCostFunction) to numer-ically check the implementation of your gradients.


You should now submit the regularized gradient function.

2.3    Learning movie recommendations

After you have nished implementing the collaborative ltering cost function and gradient, you can now start training your algorithm to make movie


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recommendations for yourself. In the next part of the ex8 cofi.m script, you can enter your own movie preferences, so that later when the algorithm runs, you can get your own movie recommendations! We have lled out some values according to our own preferences, but you should change this according to your own tastes. The list of all movies and their number in the dataset can be found listed in the le movie idx.txt.


2.3.1    Recommendations


Top recommendations for you:

Predicting rating 9.0 for movie Titanic (1997)

Predicting rating 8.9 for movie Star Wars (1977)

Predicting rating 8.8 for movie Shawshank Redemption, The (1994)

Predicting rating 8.5 for movie As Good As It Gets (1997)

Predicting rating 8.5 for movie Good Will Hunting (1997)

Predicting rating 8.5 for movie Usual Suspects, The (1995)

Predicting rating 8.5 for movie Schindler’s List (1993)

Predicting rating 8.4 for movie Raiders of the Lost Ark (1981)

Predicting rating 8.4 for movie Empire Strikes Back, The (1980)

Predicting rating 8.4 for movie Braveheart (1995)

Original ratings provided:

Rated 4 for Toy Story (1995)

Rated 3 for Twelve Monkeys (1995)

Rated 5 for Usual Suspects, The (1995)

Rated 4 for Outbreak (1995)

Rated 5 for Shawshank Redemption, The (1994)

Rated 3 for While You Were Sleeping (1995)

Rated 5 for Forrest Gump (1994)

Rated 2 for Silence of the Lambs, The (1991)

Rated 4 for Alien (1979)

Rated 5 for Die Hard 2 (1990)

Rated 5 for Sphere (1998)



Figure 4: Movie recommendations

After the additional ratings have been added to the dataset, the script will proceed to train the collaborative ltering model. This will learn the parameters X and Theta. To predict the rating of movie i for user j, you need

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to compute ( (j))T x(i). The next part of the script computes the ratings for all the movies and users and displays the movies that it recommends (Figure 4), according to ratings that were entered earlier in the script. Note that you might obtain a di erent set of the predictions due to di erent random initializations.


Submission and Grading

After completing various parts of the assignment, be sure to use the submit function system to submit your solutions to our servers. The following is a breakdown of how each part of this exercise is scored.

Part
Submitted File
Points



Estimate Gaussian Parameters
estimateGuassian.m
15 points
Select Threshold
selectThreshold.m
15 points



Collaborative Filtering Cost
cofiCostFunc.m
20 points
Collaborative Filtering Gradient
cofiCostFunc.m
30 points
Regularized Cost
cofiCostFunc.m
10 points
Gradient with regularization
cofiCostFunc.m
10 points



Total Points

100 points




You are allowed to submit your solutions multiple times, and we will take only the highest score into consideration. To prevent rapid- re guessing, the system enforces a minimum of 5 minutes between submissions.

























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