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Precision Parameter Hyperpriors

As we are employing a fully Bayesian approach we do not assume predetermined or known values for precisions in the model. Thus far in the noise modelling, these include the noise precision $ \phi _{\epsilon _i}$, the MRF parameter $ \phi _{\alpha _p}$, the ARD precisions $ \phi _{\beta _{ij}}$ and $ \phi _{\alpha _{pi}}$. We use a standard conjugate Gamma hyperprior. For the noise precision we have:
$\displaystyle \phi_{\epsilon_i}\vert \tilde{a}_{\epsilon}, \tilde{b}_{\epsilon} \sim
Ga(\tilde{a}_{\epsilon}, \tilde{b}_{\epsilon})$     (16)

for the MRF precisions:
$\displaystyle \phi_{\beta}\vert \tilde{a}_{\beta},
\tilde{b}_{\beta} \sim
Ga(\tilde{a}_{\beta}, \tilde{b}_{\beta})$      
$\displaystyle \phi_{\alpha_p}\vert \tilde{a}_{\alpha}, \tilde{b}_{\alpha} \sim
Ga(\tilde{a}_{\alpha}, \tilde{b}_{\alpha})$     (17)

and for the ARD precisions:
$\displaystyle \phi_{\beta_{ij}}\vert \tilde{a}_{\beta}, \tilde{b}_{\beta} \sim Ga(\tilde{a}_{\beta}, \tilde{b}_{\beta})$      
$\displaystyle \phi_{\alpha_{pi}}\vert \tilde{a}_{\alpha}, \tilde{b}_{\alpha} \sim
Ga(\tilde{a}_{\alpha}, \tilde{b}_{\alpha})$     (18)

where $ Ga(a_{\phi},b_{\phi})$ is the Gamma distribution, and the $ a_{\phi}$ and $ b_{\phi}$ are known hyperparameters of the Gamma distribution. Setting $ a_{\phi}=0$ and $ b_{\phi}=0$ would be equivalent to a uniform prior $ log(\sigma^2 = 1/\phi) \sim U(-\infty,+\infty)$, which would be problematic since it would result in an improper posterior with an infinite spike at $ \sigma=0$. As long as $ a_{\phi}$ and $ b_{\phi}$ are set positive then a proper posterior will result. With no prior information about the variance, $ a_{\phi}$ and $ b_{\phi}$ the approach taken is to choose a very disperse prior, i.e. with mean based on an empirical initial estimate and a very large variance so that the choice of mean hardly affects the posterior distribution.
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Next: Signal Modelling Up: Small Scale Variation Previous: Automatic Relevance Determination (ARD)