function c = tapas_logrt_linear_whatworld_config
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
% Contains the configuration for the linear log-reaction time response model according to as
% developed with Louise Marshall and Sven Bestmann
%
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
%
% The Gaussian noise observation model assumes that responses have a Gaussian distribution around
% the inferred mean of the relevant state. The only parameter of the model is the noise variance
% (NOT standard deviation) zeta.
%
% --------------------------------------------------------------------------------------------------
% Copyright (C) 2014 Christoph Mathys, UZH & ETHZ
%
% This file is part of the HGF toolbox, which is released under the terms of the GNU General Public
% Licence (GPL), version 3. You can redistribute it and/or modify it under the terms of the GPL
% (either version 3 or, at your option, any later version). For further details, see the file
% COPYING or .
% Config structure
c = struct;
% Model name
c.model = 'Linear log-reaction time for WhatWorld models';
% Sufficient statistics of Gaussian parameter priors
%
% Beta_0
c.be0mu = log(500);
c.be0sa = 4;
% Beta_1
c.be1mu = 0;
c.be1sa = 4;
% Beta_2
c.be2mu = 0;
c.be2sa = 4;
% Beta_3
c.be3mu = 0;
c.be3sa = 4;
% Zeta
c.logzemu = log(log(20));
c.logzesa = log(2);
% Gather prior settings in vectors
c.priormus = [
c.be0mu,...
c.be1mu,...
c.be2mu,...
c.be3mu,...
c.logzemu,...
];
c.priorsas = [
c.be0sa,...
c.be1sa,...
c.be2sa,...
c.be3sa,...
c.logzesa,...
];
% Model filehandle
c.obs_fun = @tapas_logrt_linear_whatworld;
% Handle to function that transforms observation parameters to their native space
% from the space they are estimated in
c.transp_obs_fun = @tapas_logrt_linear_whatworld_transp;
return;