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[ascl:2203.021] MG-MAMPOSSt: Test gravity with the mass profiles of galaxy clusters

MG-MAMPOSSt extends the MAMPOSSt code (ascl:2203.020), which performs Bayesian fits of models of mass and velocity anisotropy profiles to the distribution of tracers in projected phase space, to handle modified gravity models and constrain its parameters. It implements two distinct types of gravity modifications: general chameleon (including $f(\mathcal{R})$ models), and beyond Horndeski gravity (Vainshtein screening). MG-MAMPOSSt efficently explores the parameter space either by computing the likelihood over a multi-dimensional grid of points or by performing a simple Metropolis-Hastings MCMC. The code requires a Fortran90 compiler or higher and makes use of the getdist package (ascl:1910.018) to plot the marginalized distributions in the MCMC mode.

Code site:
https://github.com/Pizzuti92/MG-MAMPOSSt
Used in:
https://ui.adsabs.harvard.edu/abs/2022MNRAS.tmp..721P
Described in:
https://ui.adsabs.harvard.edu/abs/2022arXiv220107194P
Bibcode:
2022ascl.soft03021P

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ascl:2203.021
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