Galaxy Cluster Mass Reconstruction Project: III. The impact of dynamical substructure on cluster mass estimates

Galaxy Cluster Mass Reconstruction Project: III. The impact of dynamical substructure on cluster mass estimates

With the advent of wide-field cosmological surveys, we are approaching samples of hundreds of thousands of galaxy clusters. While such large numbers will help reduce statistical uncertainties, the control of systematics in cluster masses is crucial. Here we examine the effects of an important source...

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Bibliographic Details
Main Authors: Old, L., Wojtak, R., Pearce, F.R., Gray, M.E., Mamon, G.A., Sifón, C., Tempel, E., Biviano, A., Yee, H.K.C., de Carvalho, R., Müller, V., Sepp, T., Skibba, R.A., Croton, D., Bamford, S.P., Power, C., von der Linden, A., Saro, A.
Format: Article
Language:English
Published: Oxford University Press 2018
Subjects:
galaxies: clusters: general ; galaxies: groups: general ; galaxies: haloes ; galaxies: kinematics and dynamics ; cosmological parameters ; large-scale structure of Universe
Online Access:https://eprints.nottingham.ac.uk/49475/

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https://eprints.nottingham.ac.uk/49475/

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