The X-ray properties of weak-lensing-selected galaxy clusters

P. A. Giles, B. J. Maughan, T. Hamana, S. Miyazaki, M. Birkinshaw, R. S. Ellis, R. Massey

Research output: Contribution to journalArticle (Academic Journal)

8 Citations (Scopus)
317 Downloads (Pure)

Abstract

We present the results of an X-ray follow-up campaign targeting 10 weak-lensing (WL)-selected galaxy clusters from a Subaru WL survey. Archival Chandra data exist for two of the clusters, and we obtain dedicated observations of the remaining eight. The WL clusters appear to fit the same scaling relation between X-ray luminosity and temperature as X-ray-selected clusters. However, when we consider the luminosity–mass relation, the WL-selected clusters appear underluminous by a factor 2.1 ± 0.5 (or, alternatively, more massive by 1.7 ± 0.3), compared to X-ray-selected clusters with X-ray-based mass estimates. By considering the effects of the centroid offset, Eddington bias, and triaxiallity, this difference can be reconciled. We use X-ray imaging data to quantify the dynamical state of the clusters and found that one of the clusters appears dynamically relaxed, and two of the clusters host a cool core, consistent with Sunyaev–Zel'dovich-effect-selected clusters. This fraction is much lower than observed in X-ray-selected cluster samples.
Original languageEnglish
Pages (from-to)3044-3059
Number of pages16
JournalMonthly Notices of the Royal Astronomical Society
Volume447
Issue number4
Early online date14 Jan 2015
DOIs
Publication statusPublished - 11 Mar 2015

Keywords

  • galaxies: clusters: general
  • cosmology: observations
  • X-rays: galaxies: clusters

Fingerprint Dive into the research topics of 'The X-ray properties of weak-lensing-selected galaxy clusters'. Together they form a unique fingerprint.

Cite this