A microwave kinetic inductance detector for the DAG telescope

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dc.authorid0000-0002-3531-9842
dc.authorid0000-0002-4744-3429
dc.authorid0000-0002-7749-7575
dc.authorid0000-0002-6990-8899
dc.authorid0000-0003-2675-3564
dc.authorid0000-0003-1894-7190
dc.authorid0000-0001-9717-5349
dc.authorid0000-0003-4196-1791
dc.authorid0000-0002-2290-5228
dc.contributor.authorGüver, Tolgaen_US
dc.contributor.authorMazin, Benjamin A.en_US
dc.contributor.authorO'Brien, Kieran S.en_US
dc.contributor.authorKay, Buraken_US
dc.contributor.authorAliş, Sinanen_US
dc.contributor.authorYelkenci, Fuat Korhanen_US
dc.contributor.authorYeşilyaprak, Cahiten_US
dc.contributor.authorYerli, Sinan Kaanen_US
dc.contributor.authorErol, Ayşeen_US
dc.contributor.authorKeskin, Onuren_US
dc.date.accessioned2016-12-28T08:38:56Z
dc.date.available2016-12-28T08:38:56Z
dc.date.issued2016
dc.departmentIşık Üniversitesi, Mühendislik Fakültesi, Makine Mühendisliği Bölümüen_US
dc.departmentIşık University, Faculty of Engineering, Department of Mechanical Engineeringen_US
dc.description.abstractWe present the details of a proposed microwave kinetic inductance detector (MKID) for the DAG (Eastern Anatolia Observatory in Turkish) telescope, DAG-MKID. The observatory will have a modern 4m size telescope that is currently under construction. Current plan to obtain the first light with the telescope is late 2019. The proposed MKID based instrument will enable astronomers to simultaneously detect photons in the relatively wide wavelength range of 4000-13500 Å with a timing accuracy of ?s and spectral resolution R = /? =10-25. With a planned field of view of approximately an arcminute, DAG-MKID will mostly be used for follow-up observations of transient or variable objects as well as a robust tool to measure photometric redshifts of a large number of galaxies or other extra-galactic objects.en_US
dc.description.versionPublisher's Versionen_US
dc.identifier.citationGüver, T., Mazin, B. A., O'Brien, K., Kay, B., Aliş, S., Yelkenci, F. K., Yeşilyaprak, C., Erol, A., Yerli, S. K. & Keskin, O. (2016). A microwave kinetic inductance detector for the DAG telescope. Paper presented at the Proceedings of SPIE - The International Society for Optical Engineering, 9915, 1-8. doi:10.1117/12.2234281en_US
dc.identifier.doi10.1117/12.2234281
dc.identifier.endpage8
dc.identifier.isbn9781510602090
dc.identifier.isbn9781510602106
dc.identifier.issn0277-786X
dc.identifier.issn1996-756X
dc.identifier.scopus2-s2.0-84992539263
dc.identifier.scopusqualityN/A
dc.identifier.startpage1
dc.identifier.urihttps://hdl.handle.net/11729/1173
dc.identifier.urihttp://dx.doi.org/10.1117/12.2234281
dc.identifier.volume9915
dc.identifier.wosWOS:000385793400081
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.indekslendigikaynakConference Proceedings Citation Index – Science (CPCI-S)en_US
dc.institutionauthorKeskin, Onuren_US
dc.institutionauthorid0000-0002-2290-5228
dc.language.isoenen_US
dc.peerreviewedYesen_US
dc.publicationstatusPublisheden_US
dc.publisherSPIEen_US
dc.relation.ispartofProceedings of SPIE - The International Society for Optical Engineeringen_US
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectInductanceen_US
dc.subjectInfrared detectorsen_US
dc.subjectObservatoriesen_US
dc.subjectEastern Anatoliaen_US
dc.subjectExtra-galacticen_US
dc.subjectField of viewsen_US
dc.subjectFollow upen_US
dc.subjectKinetic inductance detectorsen_US
dc.subjectRed shiften_US
dc.subjectTurkishsen_US
dc.subjectWavelength rangesen_US
dc.subjectTelescopesen_US
dc.subjectPhotometric redshiftsen_US
dc.subjectGalaxy Clusteren_US
dc.subjectArconsen_US
dc.subjectFocal plane instrumentationen_US
dc.subjectMicrowave kinetic inductanceen_US
dc.titleA microwave kinetic inductance detector for the DAG telescopeen_US
dc.typeConference Objecten_US
dspace.entity.typePublication

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