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LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content

descriptionPublicationkeyboard_double_arrow_right Article , Preprint 05 Jan 2019Embargo end date: 01 Jan 2019 France, Italy, Finland English Publisher:Oxford University Press (OUP)Journal:Monthly Notices of the Royal Astronomical Society, volume 484, pages 60-80 (issn: 0035-8711, eissn: 1365-2966, Copyright policy )Funded by:NSF | Collaborative Research: A...
Authors: Sarah L Mulroy; Arya Farahi; August E Evrard; Graham P Smith; Alexis Finoguenov; Christine O’Donnell; Daniel P Marrone; +9 Authors

doi: 10.1093/mnras/sty3484 , 10.48550/arxiv.1901.11276

arXiv: 1901.11276

handle: 10138/308476 , 21.11116/0000-0003-735B-6 , 21.11116/0000-0003-735D-4 , 2108/250863

LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content

Abstract

We present a simultaneous analysis of galaxy cluster scaling relations between weak-lensing mass and multiple cluster observables, across a wide range of wavelengths, that probe both gas and stellar content. Our new hierarchical Bayesian model simultaneously considers the selection variable alongside all other observables in order to explicitly model intrinsic property covariance and account for selection effects. We apply this method to a sample of 41 clusters at $0.15

21 pages, 9 figures

Countries
France, Italy, Finland
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Keywords

galaxies: clusters: intracluster medium, Cosmology and Nongalactic Astrophysics (astro-ph.CO), FOS: Physical sciences, Astronomy, Space science, Settore FIS/05 - ASTRONOMIA E ASTROFISICA, Cosmology: observation, HOT GAS, gravitational lensing: weak, Gravitational lensing: weak, LINEAR-REGRESSION, Cosmology: observations; Galaxies: clusters: general; Galaxies: clusters: intracluster medium; Galaxies: stellar content; Gravitational lensing: weak, Galaxies: stellar content, 520, CHANDRA SAMPLE, EVOLUTION, SIMULATIONS, K-BAND PROPERTIES, SCATTER, galaxies: clusters: general, LUMINOSITY FUNCTION, cosmology: observations, COSMOLOGY, galaxies: stellar content, Galaxies: clusters: general, [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph], SKY, Galaxies: clusters: intracluster medium, Astrophysics - Cosmology and Nongalactic Astrophysics

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    selected citations
    These citations are derived from selected sources.
    This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 55
    popularity
    This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
    		 Top 10%
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
    		 Top 10%
    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
55
Top 10%
Top 10%
Top 10%
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gold
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