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GroundBIRD: Observing Cosmic Microwave Polarization at Large Angular Scale with Kinetic Inductance Detectors and High-Speed Rotating Telescope

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dc.contributor.authorOguri, S.-
dc.contributor.authorChoi, J.-
dc.contributor.authorDamayanthi, T.-
dc.contributor.authorHattori, M.-
dc.contributor.authorHazumi, M.-
dc.contributor.authorIshitsuka, H.-
dc.contributor.authorKaratsu, K.-
dc.contributor.authorMima, S.-
dc.contributor.authorMinowa, M.-
dc.contributor.authorNagasaki, T.-
dc.contributor.authorOtani, C.-
dc.contributor.authorSekimoto, Y.-
dc.contributor.authorTajima, O.-
dc.contributor.authorTomita, N.-
dc.contributor.authorYoshida, M.-
dc.contributor.authorWon, E.-
dc.date.accessioned2021-09-03T21:26:36Z-
dc.date.available2021-09-03T21:26:36Z-
dc.date.created2021-06-18-
dc.date.issued2016-08-
dc.identifier.issn0022-2291-
dc.identifier.urihttps://scholar.korea.ac.kr/handle/2021.sw.korea/87923-
dc.description.abstractCosmic microwave background (CMB) is an important source of information about the origin of our universe. In particular, odd-parity large angular scale patterns in the CMB polarization, the primordial B-modes, are strong evidence for an inflationary universe, related to the accelerating expansion of the metric. We are developing a unique telescope, GroundBIRD, to take CMB polarization measurements. The telescope combines novel techniques: high-speed rotation scanning, cold optics, and microwave kinetic inductance detectors (MKIDs). We evaluated the response of MKIDs on the rotation stage. Method of shielding from the geo-magnetic field is established. We have also developed a receiver cryostat. We are able to maintain a sufficient cold status for observations on the optical configuration. We plan to start commissioning the system by observing CMB in Japan in 2015-2016. We will then deploy GroundBIRD in the Canary Islands for further scientific observations.-
dc.languageEnglish-
dc.language.isoen-
dc.publisherSPRINGER/PLENUM PUBLISHERS-
dc.subjectPOWER SPECTRA-
dc.titleGroundBIRD: Observing Cosmic Microwave Polarization at Large Angular Scale with Kinetic Inductance Detectors and High-Speed Rotating Telescope-
dc.typeArticle-
dc.contributor.affiliatedAuthorWon, E.-
dc.identifier.doi10.1007/s10909-015-1420-9-
dc.identifier.scopusid2-s2.0-84952649213-
dc.identifier.wosid000379022700040-
dc.identifier.bibliographicCitationJOURNAL OF LOW TEMPERATURE PHYSICS, v.184, no.3-4, pp.786 - 792-
dc.relation.isPartOfJOURNAL OF LOW TEMPERATURE PHYSICS-
dc.citation.titleJOURNAL OF LOW TEMPERATURE PHYSICS-
dc.citation.volume184-
dc.citation.number3-4-
dc.citation.startPage786-
dc.citation.endPage792-
dc.type.rimsART-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaPhysics-
dc.relation.journalWebOfScienceCategoryPhysics, Applied-
dc.relation.journalWebOfScienceCategoryPhysics, Condensed Matter-
dc.subject.keywordPlusPOWER SPECTRA-
dc.subject.keywordAuthorCosmic microwave background-
dc.subject.keywordAuthorPolarization-
dc.subject.keywordAuthorMicrowave kinetic inductance detector-
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