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

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Mulroy , S L , Farahi , A , Evrard , A E , Smith , G P , Finoguenov , A , O'Donnell , C , Marrone , D P , Abdulla , Z , Bourdin , H , Carlstrom , J E , Democles , J , Haines , C P , Martino , R , Mazzotta , P , McGee , S L & Okabe , N 2019 , ' LoCuSS : scaling relations between galaxy cluster mass, gas, and stellar content ' , Monthly Notices of the Royal Astronomical Society , vol. 484 , no. 1 , pp. 60-80 . https://doi.org/10.1093/mnras/sty3484

Title: LoCuSS : scaling relations between galaxy cluster mass, gas, and stellar content
Author: Mulroy, Sarah L.; Farahi, Arya; Evrard, August E.; Smith, Graham P.; Finoguenov, Alexis; O'Donnell, Christine; Marrone, Daniel P.; Abdulla, Zubair; Bourdin, Herve; Carlstrom, John E.; Democles, Jessica; Haines, Chris P.; Martino, Rossella; Mazzotta, Pasquale; McGee, Sean L.; Okabe, Nobuhiro
Contributor organization: Department of Physics
Date: 2019-03
Language: eng
Number of pages: 21
Belongs to series: Monthly Notices of the Royal Astronomical Society
ISSN: 0035-8711
DOI: https://doi.org/10.1093/mnras/sty3484
URI: http://hdl.handle.net/10138/308476
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 <z <0.30, with a well-defined selection criteria based on RASS X-ray luminosity, and observations from Chandra/XMM, SZA, Planck, UKIRT, SUSS, and Subaru. These clusters have well-constrained weak-lensing mass measurements based on Subaru/SuprimeCam observations, which serve as the reference masses in our model. We present 30 scaling relation parameters for 10 properties. All relations probing the intracluster gas are slightly shallower than self-similar predictions, in moderate tension with prior measurements, and the stellar fraction decreases with mass. K-band luminosity has the lowest intrinsic scatter with a 95th percentile of 0.16, while the lowest scatter gas probe is gas mass with a fractional intrinsic scatter of 0.16 +/- 0.03. We find no distinction between the core-excised X-ray or high-resolution Sunyaev-Zel'dovich relations of clusters of different central entropy, but find with modest significance that higher entropy clusters have higher stellar fractions than their lower entropy counterparts. We also report posterior mass estimates from our likelihood model.
Subject: gravitational lensing: weak
galaxies: clusters: general
galaxies: clusters: intracluster medium
galaxies: stellar content
cosmology: observations
K-BAND PROPERTIES
LUMINOSITY FUNCTION
LINEAR-REGRESSION
CHANDRA SAMPLE
HOT GAS
SKY
EVOLUTION
SIMULATIONS
COSMOLOGY
SCATTER
115 Astronomy, Space science
Peer reviewed: Yes
Rights: cc_by_nc_sa
Usage restriction: openAccess
Self-archived version: publishedVersion


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