arXiv · 1911.04917
KISS: a spectrometric imager for millimetre cosmology
Abstract
Clusters of galaxies are used to map the large-scale structures in the universe and as probe of universe evolution. They can be observed through the Sunyaev-Zel'dovich (SZ) effect. At this respect the spectro-imaging at low resolution frequency is an important tool, today, for the study of cluster of galaxies. We have developed KISS (KIDs-Interferometer-Spectrum-Survey), a spectrometric imager dedicated to the secondary anisotropies of the Cosmic Microwave Background (CMB). The multi-frequency approach permits to improve the component separation with respect to predecessor experiments. In this paper, firstly, we provide a description of the scientific context and the state of the art of SZ observations. Secondly, we describe the KISS instrument. Finally, we show preliminary results of the ongoing commissioning campaign.
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A. Fasano, M. Aguiar, A. Benoit, A. Bideaud, O. Bourrion, M. Calvo, A. Catalano, A. P. de Taoro, G. Garde, A. Gomez, M. F. Gomez Renasco, J. Goupy, C. Hoarau, R. Hoyland, J. F. Macías-Pérez, J. Marpaud, A. Monfardini, G. Pisano, N. Ponthieu, J. A. Rubiño Martín, D. Tourres, C. Tucker, A. Beelen, G. Bres, M. De Petris, P. de Bernardis, G. Lagache, M. Marton, R. Rebolo, S. Roudier. 2019-11-12. KISS: a spectrometric imager for millimetre cosmology. https://doi.org/10.1051/epjconf%2F202022800010
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