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Follow-up of eROSITA and Euclid Galaxy Clusters with XMM-Newton

Published 16 Jan 2017 in astro-ph.CO, astro-ph.GA, and astro-ph.HE | (1701.04216v1)

Abstract: A revolution in galaxy cluster science is only a few years away. The survey machines eROSITA and Euclid will provide cluster samples of never-before-seen statistical quality. XMM-Newton will be the key instrument to exploit these rich datasets in terms of detailed follow-up of the cluster hot gas content, systematically characterizing sub-samples as well as exotic new objects.

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Authors (1)

  1. Thomas H. Reiprich 

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