A Late w-M Transition Dark Energy Model Constrained by MontePython

This project is a follow up work in which we constrain the Late w-M Transition Dark Energy model modifying MontePython, a program that performs MCMC calculations in order to calculate the best fit values of the parameters. For this purpose we substitute the default background.c, input.c and background.h files with the ones that are included in the github repository.

Code