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Galaxy cluster cosmology from X-ray surveys of the hot and energetic Universe

Published online by Cambridge University Press:  27 October 2016

Nicolas Clerc ,
Barbara Sartoris ,
Klaus Dolag ,
Rukmani Vijayaraghavan  and
Veronica Biffi
Nicolas Clerc
Affiliation:
Max-Planck Institut für extraterrestrische Physik, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
Barbara Sartoris
Affiliation:
Dipartimento di Fisica, Sezione di Astronomia, Universitá di Trieste, Via Tiepolo 11, I-34143 Trieste, Italy INAF/Osservatorio Astronomico di Trieste, Via Tiepolo 11, I-34143 Trieste, Italy
Klaus Dolag
Affiliation:
Universitäts-Sternwarte München, Scheinerstrasse 1, 81679 München, Germany
Rukmani Vijayaraghavan
Affiliation:
Department of Astronomy, University of Virginia, 530 McCormick Road Charlottesville, VA 22904, USA
Veronica Biffi
Affiliation:
Dipartimento di Fisica, Sezione di Astronomia, Universitá di Trieste, Via Tiepolo 11, I-34143 Trieste, Italy INAF/Osservatorio Astronomico di Trieste, Via Tiepolo 11, I-34143 Trieste, Italy
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Abstract

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We discuss recent advances and prospects in our understanding of the formation of structures on cosmic scales based on surveys of galaxy clusters in the X-ray bands. We highlight the interaction between observations and numerical simulations of the X-ray sky. We show how future surveys will unveil the nature of the dark energy and study its evolution with time.

Keywords

Cosmology: observationscosmology: theorylarge-scale structure of universegalaxies: clusters: generalX-rays: galaxies: clusterssurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 79 - 90
Copyright
Copyright © International Astronomical Union 2016 

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