Mercurial > hg > camir-aes2014
annotate toolboxes/distance_learning/mlr/distance/setDistanceFull.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 |
rev | line source |
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wolffd@0 | 1 function D = setDistanceFull(X, W, Ifrom, Ito) |
wolffd@0 | 2 % |
wolffd@0 | 3 % D = setDistanceFull(X, W, Ifrom, Ito) |
wolffd@0 | 4 % |
wolffd@0 | 5 % X = d-by-n data matrix |
wolffd@0 | 6 % W = d-by-d PSD matrix |
wolffd@0 | 7 % Ifrom = k-by-1 vector of source points |
wolffd@0 | 8 % Ito = j-by-1 vector of destination points |
wolffd@0 | 9 % |
wolffd@0 | 10 % D = n-by-n matrix of squared euclidean distances from Ifrom to Ito |
wolffd@0 | 11 % D is sparse, and only the rows corresponding to Ifrom and |
wolffd@0 | 12 % columns corresponding to Ito are populated. |
wolffd@0 | 13 |
wolffd@0 | 14 [d,n] = size(X); |
wolffd@0 | 15 [vecs,vals] = eig(0.5 * (W + W')); |
wolffd@0 | 16 L = real(abs(vals)).^0.5 * vecs'; |
wolffd@0 | 17 |
wolffd@0 | 18 Vfrom = L * X(:,Ifrom); |
wolffd@0 | 19 |
wolffd@0 | 20 if nargin == 4 |
wolffd@0 | 21 Vto = L * X(:,Ito); |
wolffd@0 | 22 else |
wolffd@0 | 23 Vto = L * X; |
wolffd@0 | 24 Ito = 1:n; |
wolffd@0 | 25 end |
wolffd@0 | 26 |
wolffd@0 | 27 D = distToFrom(n, Vto, Vfrom, Ito, Ifrom); |
wolffd@0 | 28 end |