We describe the preliminary on-sky results of the KIDs Interferometer Spectrum Survey (KISS), a spectral imager with a 1 deg field of view (FoV). The instrument operates in the range 120–180 GHz from the 2.25m Q-U-I JOint TEnerife telescope in Teide Observatory (Tenerife, Canary Islands), at 2 395m altitude above sea level. Spectra at low resolution, up to 1.45 GHz, are obtained using a fast (3.72 Hz mechanical frequency) Fourier transform spectrometer, coupled to a continuous dilution cryostat with a stabilized temperature of 170mK that hosts two 316-pixel arrays of lumped-element kinetic inductance detectors. KISS generates more than 3 000 spectra per second during observations and represents a pathfinder to demonstrate the potential for spectral mapping with large FoV.We give an overall description of the spectral mapping paradigm and we present recent results from observations, in this paper.
Observations with KIDs Interferometer Spectrum Survey (KISS) / Fasano, A.; Catalano, A.; Macías-Pérez, J. F.; Aguiar, M.; Beelen, A.; Benoit, A.; Bideaud, A.; Bounmy, J.; Bourrion, O.; Bres, G.; Calvo, M.; Castro-Almazán, J. A.; de Bernardis, P.; De Petris, M.; de Taoro, A. P.; Fernández-Torreiro, M.; Garde, G.; Génova-Santos, R.; Gomez, A.; Gómez-Renasco, M. F.; Goupy, J.; Hoarau, C.; Hoyland, R.; Lagache, G.; Marpaud, J.; Marton, M.; Monfardini, A.; Peel, M. W.; Pisano, G.; Ponthieu, N.; Rebolo, R.; Roudier, S.; Rubiño-Martín, J. A.; Tourres, D.; Tucker, C.; Vescovi, and C.. - In: EPJ WEB OF CONFERENCES. - ISSN 2101-6275. - 257:(2022). (Intervento presentato al convegno mm Universe @ NIKA2 - Observing the mm Universe with the NIKA2 camera tenutosi a Rome) [10.1051/epjconf/202225700017].
Observations with KIDs Interferometer Spectrum Survey (KISS)
P. de Bernardis;M. De Petris;G. Pisano;
2022
Abstract
We describe the preliminary on-sky results of the KIDs Interferometer Spectrum Survey (KISS), a spectral imager with a 1 deg field of view (FoV). The instrument operates in the range 120–180 GHz from the 2.25m Q-U-I JOint TEnerife telescope in Teide Observatory (Tenerife, Canary Islands), at 2 395m altitude above sea level. Spectra at low resolution, up to 1.45 GHz, are obtained using a fast (3.72 Hz mechanical frequency) Fourier transform spectrometer, coupled to a continuous dilution cryostat with a stabilized temperature of 170mK that hosts two 316-pixel arrays of lumped-element kinetic inductance detectors. KISS generates more than 3 000 spectra per second during observations and represents a pathfinder to demonstrate the potential for spectral mapping with large FoV.We give an overall description of the spectral mapping paradigm and we present recent results from observations, in this paper.| File | Dimensione | Formato | |
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Fasano_Observations with KIDs_2021.pdf
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Note: https://www.epj-conferences.org/articles/epjconf/abs/2022/01/epjconf_mmUniverse2021_00017/epjconf_mmUniverse2021_00017.html
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