Software Open Access

MW Satellite LF: v1.0.0

Newton, Oliver; Cautun, Marius

Initial public release of a code to calculate the luminosity function of Milky Way (MW) satellite galaxies using Approximate Bayesian Computation. The analysis uses as input only the observed satellite galaxies in the Sloan Digital Sky Survey (SDSS) and Dark Energy Survey (DES), and five Dark Matter-only simulations of MW-like haloes from the Aquarius simulation suite (Aq-A - Aq-E). Input data of the correct format is supplied for all known confirmed and candidate satellite galaxies as of February 2018.

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Publication date:
March 22, 2018
DOI:
10.5281/zenodo.1205622

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10.5281/zenodo.1205622

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Keyword(s):
Dark Matter Galaxies: dwarf Galaxy: halo
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License (for files):
GNU General Public License v3.0 only

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Version v1.0.0 10.5281/zenodo.1205622 Mar 22, 2018
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