Cosmography and Large Scale Structure by -Gravity: New Results
Figure 5
(a) histogram of the sample points for parameter in Abell 383 coming out the MCMC implementation used to estimate best fit values and errors for our fitting procedure as described in Section 11.5. Binning (horizontal axis) and relative frequencies (vertical axis) are given by automatic procedure from Mathematica6.0. (b) power spectrum test on sample chain for parameter using the method described in Section 11.5. Black line is the logarithm of the analytical template (146) for power spectrum; gray line is the discrete power spectrum obtained using (144)–(145).
