Cosmological results from the BOSS final data release
I would like to present two papers we have just submitted (arXiv:1607.03151 and arXiv:1607.03152). They are part of a set that analyses the final galaxy clustering dataset from BOSS. One is focusing on the methodology of speeding up the computation of the Markov Chain Marte Carlo analysis when using an advance/slow theoretical model; the other one is presenting an analysis considering the cosmic microwave background and the observed three-dimensional galaxy distribution to derive cosmological parameters with minimum assumptions. Our results can be used to test different dark energy models. In addition, we extend our study to measure neutrino masses given different dark energy models.