Mapping Galaxy Clusters in the Distant Universe. (arXiv:1903.06238v1 [astro-ph.GA])

Mapping Galaxy Clusters in the Distant Universe. (arXiv:1903.06238v1 [astro-ph.GA])
<a href="http://arxiv.org/find/astro-ph/1/au:+Dannerbauer_H/0/1/0/all/0/1">H. Dannerbauer</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kampen_E/0/1/0/all/0/1">E. van Kampen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Afonso_J/0/1/0/all/0/1">J. Afonso</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Andreani_P/0/1/0/all/0/1">P. Andreani</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Battaia_F/0/1/0/all/0/1">F. Arrigoni Battaia</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Bertoldi_F/0/1/0/all/0/1">F. Bertoldi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Casey_C/0/1/0/all/0/1">C. Casey</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Chen_C/0/1/0/all/0/1">C.-C. Chen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Clements_D/0/1/0/all/0/1">D. L. Clements</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Breuck_C/0/1/0/all/0/1">C. De Breuck</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Frye_B/0/1/0/all/0/1">B. Frye</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Geach_J/0/1/0/all/0/1">J. Geach</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Harrington_K/0/1/0/all/0/1">K. Harrington</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Hayashi_M/0/1/0/all/0/1">M. Hayashi</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Jin_S/0/1/0/all/0/1">S. Jin</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Klaassen_P/0/1/0/all/0/1">P. Klaassen</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Kohno_K/0/1/0/all/0/1">K. Kohno</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Lehnert_M/0/1/0/all/0/1">M. D. Lehnert</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Matute_I/0/1/0/all/0/1">I. Matute</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Mroczkowski_T/0/1/0/all/0/1">T. Mroczkowski</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Noble_A/0/1/0/all/0/1">A. Noble</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Pappalardo_C/0/1/0/all/0/1">C. Pappalardo</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tamura_Y/0/1/0/all/0/1">Y. Tamura</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Zavala_J/0/1/0/all/0/1">J. Zavala</a>

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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