KISS: a spectrometric imager for millimetre cosmology
arXiv:1911.04917 · doi:10.1051/epjconf/202022800010
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.
arXiv commentTo appear in the proceedings of the international conference entitled mm Universe @ NIKA2, Grenoble (France), June 2019, EPJ Web of conferences
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Cited by in corpus (4)
- A wide field-of-view low-resolution spectrometer at APEX: instrument design and science forecast
- Applications for Microwave Kinetic Induction Detectors in Advanced Instrumentation
- Accurate sky signal reconstruction for ground-based spectroscopy with kinetic inductance detectors
- Observations with KIDs Interferometer Spectrum Survey(KISS)