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The KISS Experiment

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dc.contributor.authorFasano, A.
dc.contributor.authorAguiar, M.
dc.contributor.authorBenoit, A.
dc.contributor.authorBideaud, A.
dc.contributor.authorBourrion, O.
dc.contributor.authorCalvo, M.
dc.contributor.authorCatalano, A.
dc.contributor.authorDe Taoro, A. P.
dc.contributor.authorGarde, G.
dc.contributor.authorGómez, A.
dc.contributor.authorGómez Reñasco, M. F.
dc.contributor.authorGoupy, J.
dc.contributor.authorHoarau, C.
dc.contributor.authorHoyland, R.
dc.contributor.authorMacías Pérez, J. F.
dc.contributor.authorMarpaud, J.
dc.contributor.authorMonfardini, A.
dc.contributor.authorPisano, G.
dc.contributor.authorPonthieu, N.
dc.contributor.authorRubiño Martín, J. A.
dc.contributor.authorTourres, D.
dc.contributor.authorTucker, C.
dc.contributor.authorBeelen, A.
dc.contributor.authorBres, G.
dc.contributor.authorDe Petris, M.
dc.contributor.authorDe Bernardis, P.
dc.contributor.authorLagache, G.
dc.contributor.authorLamagna, L.
dc.contributor.authorLuzzi, G.
dc.contributor.authorMarton, M.
dc.contributor.authorMasi, S.
dc.contributor.authorRebolo, R.
dc.contributor.authorRoudier, S.
dc.contributor.orcidDe Petris, M. [0000-0001-7859-2139]
dc.contributor.orcidMarcías Pérez, J. F. [0000-0002-5385-2763]
dc.contributor.orcidGómez, A. [0000-0002-8752-1401]
dc.contributor.orcidFasano, A. [0000-0003-4041-418X]
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
dc.date.accessioned2021-04-12T09:51:15Z
dc.date.available2021-04-12T09:51:15Z
dc.date.issued2020-04-10
dc.descriptionSpringer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.es
dc.description.abstractMapping millimetre continuum emission has become a key issue in modern multi-wavelength astrophysics. In particular, spectrum imaging at low-frequency resolution is an asset for characterising the clusters of galaxies via the Sunyaev-Zel'dovich effect. In this context, we have built a ground-based spectrum-imager named KIDs Interferometer Spectrum Survey (KISS). This instrument is based on two 316-pixel arrays of Kinetic Inductance Detectors (KID) cooled to 150 mK by a custom dilution refrigerator-based cryostat. By using Ti-Al and Al absorbers, we can cover a wide frequency range between 80 and 300 GHz. In order to preserve a large instantaneous field of view similar to 1 circle the spectrometer is based on a Fourier transform interferometer. This represents a technological challenge due to the fast scanning speed that is needed to overcome the effects of background atmospheric fluctuations. KISS is installed at the QUIJOTE 2.25 m telescope in Tenerife since February 2019 and is currently in its commissioning phase. In this report, we present an overview of the instrument and the latest results.es
dc.description.peerreviewedPeer reviewes
dc.description.sponsorshipWith funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737)es
dc.identifier.citationJournal of Low Temperature Physics 199(1-2): 529–536(2020)es
dc.identifier.doi10.1007/s10909-019-02289-1
dc.identifier.e-issn1573-7357
dc.identifier.issn0022-2291
dc.identifier.otherhttps://link.springer.com/article/10.1007/s10909-019-02289-1
dc.identifier.urihttp://hdl.handle.net/20.500.12666/232
dc.language.isoenges
dc.publisherSpringer Linkes
dc.rights.accessRightsinfo:eu-repo/semantics/restrictedAccess
dc.rights.licenseCopyright © 2019, Springer Science Business Media, LLC, part of Springer Nature
dc.subjectKinetic inductance detectorses
dc.subjectFourier transform spectroscopyes
dc.subjectSunyaev-Zel´dovich effectes
dc.titleThe KISS Experimentes
dc.typeinfo:eu-repo/semantics/articlees
dc.type.coarhttp://purl.org/coar/resource_type/c_6501
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion
dspace.entity.typePublication

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