KISS: a spectrometric imager for millimetre cosmology

Bibcode
2020EPJWC.22800010F
DOI
10.1051/epjconf/202022800010
Fasano, A.; Aguiar, M.; Benoit, A.; Bideaud, A.; Bourrion, O.; Calvo, M.; Catalano, A.; de Taoro, A. P.; Garde, G.; Gomez, A.; Gomez Renasco, M. F.; Goupy, J.; Hoarau, C.; Hoyland, R.; Macías-Pérez, J. F.; Marpaud, J.; Monfardini, A.; Pisano, G.; Ponthieu, N.; Rubiño Martín, J. A.; Tourres, D.; Tucker, C.; Beelen, A.; Bres, G.; De Petris, M.; de Bernardis, P.; Lagache, G.; Marton, M.; Rebolo, R.; Roudier, S.
Referencia bibliográfica

European Physical Journal Web of Conferences

Advertised on:
6
2020
Número de autores
30
Número de autores del IAC
8
Número de citas
2
Número de citas referidas
1
Descripción
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. In 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.
Tipo
Sin árbitro

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