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CPS2101 Bertail Patrice et al.
from the Gamma distribution Γ(1,1) and the rays W.1 and W.2 are defined by the
angles α1 = π/12 and α2 = π/3 they respectively form with the v1-axis. Fig. below
shows the related data cloud together with the log-likelihood surface
evaluated on a grid of 21x21, between [0,π/2], for (α1,α2): ML estimates
coincide with the generating W.
The model selection is illustrated by Fig. 2, for the same type of model as
previously, except that F = 10 and K = 5. The model selection procedure allows
to recover the true dimension.
5. Conclusions
In this paper we have formulated the NMF as a statistical problem. For
different generative models, identifiabilty of the related statistical models have
been investigated from a semi-parametric angle. A semi-parametric statistical
framework have been then proposed, where the proposed Z-estimator is
asymptotically consistent. Finally, we have shown how to use information
criteria such as BIC or AIC for parametric model selection purposes in the NMF
context.
Figure 1: A 2 −d NMF toy example: cone and likelihood.
18.75
AIC
18.7 BIC
18.65
18.6
18.55
18.5
18.45
18.4
18.35
2 4 6 8 10
K
Figure 2: Information criteria (AIC and BIC) as a function of the cone dimension.
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