Probing dark energy via galaxy cluster outskirts
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/457/3/3266/8001204/stw143.pdf
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3. The X-ray surface brightness profiles of hot galaxy clusters up to $\vec z$ ~ 0.8: Evidence for self-similarity and constraints on $\Omega_\mathsf{0}$
4. The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and theYSZ–M500relation
5. The Chemical Composition of the Sun
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