---
res:
  bibo_abstract:
  - An extensive sample of galaxy clusters will be available in the coming years,
    detected through their Sunyaev-Zeldovich effect (SZE). We use a semianalytic model
    to study the scientific yield of combining SZE data with X-ray and optical follow-up
    observations. If clusters at a given redshift z0 can be identified with virialized,
    spherical halos, they populate a well-defined "fundamental plane" (FP) in the
    parameter space of the three observables virial temperature (T), total Sunyaev-Zeldovich
    flux decrement (ΔSν), and angular size (θ). The location and orientation of the
    FP, as well as its redshift evolution, are sensitive to both the internal evolution
    of clusters and to the underlying cosmological parameters. We show that if clusters
    are not standard candles (e.g., because of feedback or energy injection), then
    this can be inferred from the FP. Likewise, we study the dependence of the FP
    on the cosmological parameters h, σ8, and Ω0, and quantify future constraints
    on these parameters. We also show that in the absence of any nongravitational
    effects, the scatter in the (ΔSν,T)-plane is significantly smaller than in either
    the (θ,T) or the (θ,ΔSν) planes. As a result, the ΔSν-T relation can be an exceptionally
    sensitive probe of both cluster physics and cosmological parameters. A comparison
    of the amount of scatter in these three scaling relations will test the origin
    (cosmological vs. stochastic) of the scatter.@eng
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Licia
      foaf_name: Verde, Licia
      foaf_surname: Verde
  - foaf_Person:
      foaf_givenName: Zoltán
      foaf_name: Haiman, Zoltán
      foaf_surname: Haiman
      foaf_workInfoHomepage: http://www.librecat.org/personId=7c006e8c-cc0d-11ee-8322-cb904ef76f36
  - foaf_Person:
      foaf_givenName: David N.
      foaf_name: Spergel, David N.
      foaf_surname: Spergel
  bibo_doi: 10.1086/344134
  bibo_issue: '1'
  bibo_volume: 581
  dct_date: 2002^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/0004-637X
  - http://id.crossref.org/issn/1538-4357
  dct_language: eng
  dct_publisher: American Astronomical Society@
  dct_title: Are clusters standard candles? Galaxy cluster scaling relations with
    the Sunyaev‐Zeldovich effect@
...