Mercurial > hg > camir-aes2014
comparison toolboxes/distance_learning/mlr/distance/setDistanceFullMKL.m @ 0:e9a9cd732c1e tip
first hg version after svn
author | wolffd |
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date | Tue, 10 Feb 2015 15:05:51 +0000 |
parents | |
children |
comparison
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-1:000000000000 | 0:e9a9cd732c1e |
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1 function D = setDistanceFullMKL(X, W, Ifrom, Ito) | |
2 % | |
3 % D = setDistanceFullMKL(X, W, Ifrom, Ito) | |
4 % | |
5 % X = d-by-n-by-m data matrix | |
6 % W = d-by-d-by-m PSD matrix | |
7 % Ifrom = k-by-1 vector of source points | |
8 % Ito = j-by-1 vector of destination points | |
9 % | |
10 % D = n-by-n matrix of squared euclidean distances from Ifrom to Ito | |
11 % D is sparse, and only the rows corresponding to Ifrom and | |
12 % columns corresponding to Ito are populated. | |
13 | |
14 [d,n,m] = size(X); | |
15 | |
16 D = 0; | |
17 | |
18 if nargin < 4 | |
19 Ito = 1:n; | |
20 end | |
21 | |
22 parfor i = 1:m | |
23 [vecs,vals] = eig(0.5 * (W(:,:,i) + W(:,:,i)')); | |
24 L = real(abs(vals)).^0.5 * vecs'; | |
25 | |
26 Vfrom = L * X(:,Ifrom,i); | |
27 | |
28 Vto = L * X(:,Ito,i); | |
29 | |
30 D = D + distToFrom(n, Vto, Vfrom, Ito, Ifrom); | |
31 end | |
32 end |