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

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.

5 pages; to appear in Astronomische Nachrichten, presented at the "XMM-Newton: The Next Decade" conference, ESAC, Madrid, Spain, 9 - 11 May 2016

References in corpus (4)

• Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
• XMM-Newton and Chandra Cross Calibration Using HIFLUGCS Galaxy Clusters: Systematic Temperature Differences and Cosmological Impact
• Constraining galaxy cluster temperatures and redshifts with eROSITA survey data
• The long X-ray tail in Zwicky 8338

Cited by in corpus (7)

• The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
• Probing cosmic isotropy with a new X-ray galaxy cluster sample through the $L_{\text{X}}-T$ scaling relation
• Cosmological implications of the anisotropy of ten galaxy cluster scaling relations
• X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton
• Anisotropy of the galaxy cluster X-ray luminosity-temperature relation
• Projection effects in galaxy cluster samples: insights from X-ray redshifts
• EROSITA Spectro-Imaging Analysis of the Abell 3408 Galaxy Cluster