Implicit Priors in Galaxy Cluster Mass and Scaling Relation Determinations
Adam Mantz (NASA/GSFC), Steven W. Allen (KIPAC, Stanford/SLAC)

TL;DR
This paper examines how fully parametric models of the intracluster medium in galaxy clusters inherently impose priors that bias mass scaling relation slopes towards the self-similar model, affecting the interpretation of observational data.
Contribution
It reveals the implicit priors in parametric ICM modeling and discusses their impact on scaling relation analyses, proposing alternative approaches to avoid bias.
Findings
Parametric models favor self-similar slope values.
Non-parametric methods do not impose such priors.
Literature shows clustering of results based on modeling approach.
Abstract
Deriving the total masses of galaxy clusters from observations of the intracluster medium (ICM) generally requires some prior information, in addition to the assumptions of hydrostatic equilibrium and spherical symmetry. Often, this information takes the form of particular parametrized functions used to describe the cluster gas density and temperature profiles. In this paper, we investigate the implicit priors on hydrostatic masses that result from this fully parametric approach, and the implications of such priors for scaling relations formed from those masses. We show that the application of such fully parametric models of the ICM naturally imposes a prior on the slopes of the derived scaling relations, favoring the self-similar model, and argue that this prior may be influential in practice. In contrast, this bias does not exist for techniques which adopt an explicit prior on the…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Climate variability and models · Stellar, planetary, and galactic studies
