학술논문
Mapping Galaxy Clusters in the Distant Universe
Document Type
Working Paper
Author
Dannerbauer, H.; van Kampen, E.; Afonso, J.; Andreani, P.; Battaia, F. Arrigoni; Bertoldi, F.; Casey, C.; Chen, C. -C.; Clements, D. L.; De Breuck, C.; Frye, B.; Geach, J.; Harrington, K.; Hayashi, M.; Jin, S.; Klaassen, P.; Kohno, K.; Lehnert, M. D.; Matute, I.; Mroczkowski, T.; Noble, A.; Pappalardo, C.; Tamura, Y.; Zavala, J.
Source
Subject
Language
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.
Comment: Science white paper submitted to the Astro2020 Decadal Survey
Comment: Science white paper submitted to the Astro2020 Decadal Survey