Dependence on supernovae light-curve processing in void models
  In this work, we show that when supernova Ia (SN Ia) data sets are used to
put constraints on the free parameters of inhomogeneous models, certain extra
information regarding the light-curve fitter used in the supernovae Ia
luminosity fluxes processing should be taken into account. We found that the
size of the void as well as other parameters of these models might be suffering
extra degenerations or additional systematic errors due to the fitter. A recent
proposal to relieve the tension between the results from Planck satellite and
SNe Ia is re-analyzed in the framework of these subjects.
