Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters to z = 1.3

Galaxy kinematics and mass calibration in massive SZE-selected galaxy clusters to z = 1.3

© 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. The galaxy phase-space distribution in galaxy clusters provides insights into the formation and evolution of cluster galaxies, and it can also be used to measure cluster mass profiles. We present...

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Bibliographic Details
Main Authors: Capasso, R., Saro, A., Mohr, J.J., Biviano, A., Bocquet, S., Strazzullo, V., Grandis, S., Applegate, D.E., Bayliss, Matthew B, Benson, B.A., Bleem, L.E., Brodwin, M., Bulbul, Esra, Carlstrom, J.E., Chiu, I., Dietrich, J.P., Gupta, N., de Haan, T., Hlavacek-Larrondo, J., Klein, M., von der Linden, A., McDonald, Michael A., Rapetti, D., Reichardt, C.L., Sharon, K., Stalder, B., Stanford, S.A., Stark, A.A., Stern, C., Zenteno, A.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:English
Published: Oxford University Press (OUP) 2022
Online Access:https://hdl.handle.net/1721.1/132490.2

Internet

https://hdl.handle.net/1721.1/132490.2

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