Mercurial > hg > camir-aes2014
view toolboxes/FullBNT-1.0.7/bnt/CPDs/@gaussian_CPD/log_prob_node.m @ 0:e9a9cd732c1e tip
first hg version after svn
author | wolffd |
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date | Tue, 10 Feb 2015 15:05:51 +0000 |
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function L = log_prob_node(CPD, self_ev, pev) % LOG_PROB_NODE Compute prod_m log P(x(i,m)| x(pi_i,m), theta_i) for node i (gaussian) % L = log_prob_node(CPD, self_ev, pev) % % self_ev(m) is the evidence on this node in case m. % pev(i,m) is the evidence on the i'th parent in case m (if there are any parents). % (These may also be cell arrays.) if iscell(self_ev), usecell = 1; else usecell = 0; end use_log = 1; ncases = length(self_ev); nparents = length(CPD.sizes)-1; assert(ncases == size(pev, 2)); if ncases == 0 L = 0; return; end L = 0; for m=1:ncases if isempty(CPD.dps) i = 1; else if usecell dpvals = cat(1, pev{CPD.dps, m}); else dpvals = pev(CPD.dps, m); end i = subv2ind(CPD.sizes(CPD.dps), dpvals(:)'); end if usecell y = self_ev{m}; else y = self_ev(m); end if length(CPD.cps) == 0 L = L + gaussian_prob(y, CPD.mean(:,i), CPD.cov(:,:,i), use_log); else if usecell x = cat(1, pev{CPD.cps, m}); else x = pev(CPD.cps, m); end L = L + gaussian_prob(y, CPD.mean(:,i) + CPD.weights(:,:,i)*x, CPD.cov(:,:,i), use_log); end end