Bayesian analysis of Friedmannless cosmologies
  Assuming only a homogeneous and isotropic universe and using both the 'Gold' Supernova Type Ia sample of Riess et al. and the results from the Supernova Legacy Survey, we calculate the Bayesian evidence of a range of different parameterizations of the deceleration parameter. We consider both spatially flat and curved models. Our results show that although there is strong evidence in the data for an accelerating universe, there is little evidence that the deceleration parameter varies with redshift. 
Oystein Elgaroy (ITA, University of Oslo) and Tuomas Multamaki   (Department of Physics, University of Turku)