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The X-Ray-Optical Relations for Nine Clusters at z = 0.7-1.1 from the ORELSE Survey

Rumbaugh, N. and Kocevski, D. D. and Gal, R. R. and Lemaux, B. C. and Lubin, L. M. and Fassnacht, C. D. and Squires, G. K. (2013) The X-Ray-Optical Relations for Nine Clusters at z = 0.7-1.1 from the ORELSE Survey. Astrophysical Journal, 763 (2). Art. No. 124. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20130222-141228689

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Abstract

We use Chandra observations of nine optically and X-ray-selected clusters in five different structures at z ~ 0.7-1.1 from the Observations of Redshift Evolution in Large-Scale Environments survey to study diffuse X-ray emission from galaxy clusters. X-ray gas temperatures and bolometric rest-frame luminosities are measured for each cluster in the sample. We present new redshift measurements, derived from data obtained using the Deep Imaging Multi-Object Spectrograph on the Keck 10 m telescope, for two clusters in the RX J0910 supercluster at z ~ 1.1, from which velocity dispersions are measured. Dispersions for all clusters are combined with X-ray luminosities and gas temperatures to evaluate how the cluster properties compare to low-redshift scaling relations. We also measure the degree of substructure in each cluster by examining the velocity histograms, performing Dressler-Shectman tests, and computing the offsets between the X-ray emission center and optically derived centroids. We find that only two clusters show clear indications of being unrelaxed, based on their scaling relations and other dynamical state diagnostics. Using our sample, we evaluate the redshift evolution of the Lx -T relation and investigate the implications of our results for precision cosmology surveys.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/763/2/124DOIUNSPECIFIED
http://iopscience.iop.org/0004-637X/763/2/124PublisherUNSPECIFIED
ORCID:
AuthorORCID
Lemaux, B. C.0000-0002-1428-7036
Fassnacht, C. D.0000-0002-4030-5461
Squires, G. K.0000-0002-1977-5717
Additional Information:© 2013 American Astronomical Society. Received 2012 June 30; accepted 2012 December 12; published 2013 January 16. This work is supported by the Chandra General Observing Program under award numbers GO6-7114X, GO7-8126X, GO8-9123A, and GO9-0139A. In addition, we acknowledge support by the National Science Foundation under grant AST- 0907858. Spectrographic data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. As always, we thank the indigenous Hawaiian community for allowing us to be guests on their sacred mountain. We are most fortunate to be able to conduct observations from this site.
Funders:
Funding AgencyGrant Number
Chandra General Observing ProgramGO6-7114X
Chandra General Observing ProgramGO7-8126X
Chandra General Observing ProgramGO8-9123A
Chandra General Observing ProgramGO9-0139A
NSFAST-0907858
W. M. Keck FoundationUNSPECIFIED
Subject Keywords:cosmology: observations; galaxies: clusters: general
Issue or Number:2
Record Number:CaltechAUTHORS:20130222-141228689
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130222-141228689
Official Citation:The X-Ray-Optical Relations for Nine Clusters at z = 0.7-1.1 from the ORELSE Survey N. Rumbaugh, D. D. Kocevski, R. R. Gal, B. C. Lemaux, L. M. Lubin, C. D. Fassnacht, and G. K. Squires doi:10.1088/0004-637X/763/2/124
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:37087
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:22 Feb 2013 22:27
Last Modified:09 Mar 2020 13:19

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