Mapping Galaxy Clusters in the Distant Universe

H. Dannerbauer; E. van Kampen; J. Afonso; P. Andreani; F. Arrigoni Battaia; F. Bertoldi; C. Casey; C. -C. Chen; D. L. Clements; C. De Breuck; B. Frye; J. Geach; K. Harrington; M. Hayashi; S. Jin; P. Klaassen; K. Kohno; M. D. Lehnert; I. Matute; T. Mroczkowski; A. Noble; C. Pappalardo; Y. Tamura; J. Zavala

arXiv · 1903.06238

Mapping Galaxy Clusters in the Distant Universe

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Abstract

We present the science case for mapping several thousand galaxy (proto)clusters at z=1-10 with a large aperture single dish sub-mm facility, producing a high-redshift counterpart to local large surveys of rich clusters like the well-studied Abell catalogue. Principal goals of a large survey of distant clusters are the evolution of galaxy clusters over cosmic time and the impact of environment on the evolution and formation of galaxies. To make a big leap forward in this emerging research field, the community would benefit from a large-format, wide-band, direct-detection spectrometer (e.g., based on MKID technology), covering a wide field of ~1 square degree and a frequency coverage from 70 to 700 GHz.

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H. Dannerbauer, E. van Kampen, J. Afonso, P. Andreani, F. Arrigoni Battaia, F. Bertoldi, C. Casey, C. -C. Chen, D. L. Clements, C. De Breuck, B. Frye, J. Geach, K. Harrington, M. Hayashi, S. Jin, P. Klaassen, K. Kohno, M. D. Lehnert, I. Matute, T. Mroczkowski, A. Noble, C. Pappalardo, Y. Tamura, J. Zavala. 2019-03-14. Mapping Galaxy Clusters in the Distant Universe. https://arxiv.org/abs/1903.06238

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