{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360004233103902848.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1017/s1743921312009672"}},{"identifier":{"@type":"URI","@value":"https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921312009672"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Cosmic Infrared Background ExpeRiment (CIBER): A probe of Extragalactic Background Light from reionization"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>The Cosmic Infrared Background ExpeRiment (CIBER) is a rocket-borne absolute photometry imaging and spectroscopy experiment optimized to detect signatures of first-light galaxies present during reionization in the unresolved IR background. CIBER-I consists of a wide-field two-color camera for fluctuation measurements, a low-resolution absolute spectrometer for absolute EBL measurements, and a narrow-band imaging spectrometer to measure and correct scattered emission from the foreground zodiacal cloud. CIBER-I was successfully flown in February 2009 and July 2010 and four more flights are planned by 2014, including an upgrade (CIBER-II). We propose, after several additional flights of CIBER-I, an improved CIBER-II camera consisting of a wide-field 30 cm imager operating in 4 bands between 0.5 and 2.1 microns. It is designed for a high significance detection of unresolved IR background fluctuations at the minimum level necessary for reionization. With a FOV 50 to 2000 times larger than existing IR instruments on satellites, CIBER-II will carry out the definitive study to establish the surface density of sources responsible for reionization.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004233103902850","@type":"Researcher","foaf:name":[{"@value":"Asantha Cooray"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902721","@type":"Researcher","foaf:name":[{"@value":"Jamie Bock"}]},{"@id":"https://cir.nii.ac.jp/crid/1420845751151554944","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"50280558"},{"@type":"NRID","@value":"1000050280558"},{"@type":"NRID","@value":"9000000121682"}],"foaf:name":[{"@value":"Mitsunobu Kawada"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902724","@type":"Researcher","foaf:name":[{"@value":"Brian Keating"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902848","@type":"Researcher","foaf:name":[{"@value":"Andrew Lange"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902851","@type":"Researcher","foaf:name":[{"@value":"Dae-Hee Lee"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902726","@type":"Researcher","foaf:name":[{"@value":"Louis Levenson"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902725","@type":"Researcher","foaf:name":[{"@value":"Toshio 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Matsuura"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902729","@type":"Researcher","foaf:name":[{"@value":"Tom Renbarger"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902722","@type":"Researcher","foaf:name":[{"@value":"Ian Sullivan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902728","@type":"Researcher","foaf:name":[{"@value":"Kohji Tsumura"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902723","@type":"Researcher","foaf:name":[{"@value":"Takehiko Wada"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004233103902849","@type":"Researcher","foaf:name":[{"@value":"Michael Zemcov"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"17439213"},{"@type":"EISSN","@value":"17439221"}],"prism:publicationName":[{"@value":"Proceedings of the International Astronomical Union"}],"dc:publisher":[{"@value":"Cambridge University Press (CUP)"}],"prism:publicationDate":"2011-09","prism:volume":"7","prism:number":"S284","prism:startingPage":"482","prism:endingPage":"488"},"reviewed":"false","dc:rights":["https://www.cambridge.org/core/terms"],"url":[{"@id":"https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921312009672"}],"createdAt":"2012-08-17","modifiedAt":"2019-04-27","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Astronomy%20and%20Astrophysics","dc:title":"Astronomy and Astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=Space%20and%20Planetary%20Science","dc:title":"Space and Planetary Science"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040282257039723264","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"21111004"},{"@type":"JGN","@value":"JP21111004"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-21111004/"}],"notation":[{"@language":"ja","@value":"宇宙赤外線背景放射の観測によるダークエイジの探査"},{"@language":"en","@value":"Exploration of the dark age by 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