{ "id": "1411.3786", "version": "v1", "published": "1970-01-01T00:00:00.000Z", "updated": "2014-11-14T04:14:54.000Z", "title": "Bayesian Analysis for Stellar Evolution with Nine Parameters (BASE-9): User's Manual", "authors": [ "Ted von Hippel", "Elliot Robinson", "Elizabeth Jeffery", "Rachel Wagner-Kaiser", "Steven DeGennaro", "Nathan Stein", "David Stenning", "William H. Jefferys", "David van Dyk" ], "comment": "22 pages, 7 figures", "categories": [ "astro-ph.SR", "astro-ph.IM" ], "abstract": "BASE-9 is a Bayesian software suite that recovers star cluster and stellar parameters from photometry. BASE-9 is useful for analyzing single-age, single-metallicity star clusters, binaries, or single stars, and for simulating such systems. BASE-9 uses Markov chain Monte Carlo and brute-force numerical integration techniques to estimate the posterior probability distributions for the age, metallicity, helium abundance, distance modulus, and line-of-sight absorption for a cluster, and the mass, binary mass ratio, and cluster membership probability for every stellar object. BASE-9 is provided as open source code on a version-controlled web server. The executables are also available as Amazon Elastic Compute Cloud images. This manual provides potential users with an overview of BASE-9, including instructions for installation and use.", "revisions": [ { "version": "v0", "updated": "1970-01-01T00:00:00.000Z", "title": "", "abstract": "", "comment": null, "journal": null, "doi": null, "authors": [] }, { "version": "v1", "updated": "2014-11-14T04:14:54.000Z" } ], "analyses": { "keywords": [ "stellar evolution", "bayesian analysis", "users manual", "parameters", "markov chain monte carlo" ], "tags": [ "manual" ], "note": { "typesetting": "TeX", "pages": 22, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014arXiv1411.3786V" } } }