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dc.contributor.authorHayton, D. J.
dc.contributor.authorKloosterman, J. L.
dc.contributor.authorRen, Y.
dc.contributor.authorGao, J. R.
dc.contributor.authorKlapwijk, T. M.
dc.contributor.authorHu, Q.
dc.contributor.authorWalker, C. K.
dc.contributor.authorReno, J. L.
dc.contributor.authorKao, T.-Y.
dc.contributor.authorHu, Qing
dc.date.accessioned2015-12-18T13:25:37Z
dc.date.available2015-12-18T13:25:37Z
dc.date.issued2014-07
dc.identifier.issn0277-786X
dc.identifier.urihttp://hdl.handle.net/1721.1/100425
dc.description.abstractWe report on the performance of a high sensitivity 4.7 THz heterodyne receiver based on a NbN hot electron bolometer mixer and a quantum cascade laser (QCL) as local oscillator. The receiver is developed to observe the astronomically important neutral atomic oxygen [OI] line at 4.7448 THz on a balloon based telescope. The single-line frequency control and improved beam pattern of QCL have taken advantage of a third-order distributed feedback structure. We measured a double sideband receiver noise temperature (T[subscript rec(DSB)]) of 815 K, which is ~ 7 times the quantum noise limit (hν/2kB). An Allan time of 15 s at an effective noise fluctuation bandwidth of 18 MHz is demonstrated. Heterodyne performance was further supported by a measured methanol line spectrum around 4.7 THz.en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administrationen_US
dc.description.sponsorshipNational Science Foundation (U.S.)en_US
dc.language.isoen_US
dc.publisherSPIEen_US
dc.relation.isversionofhttp://dx.doi.org/10.1117/12.2055790en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceSPIEen_US
dc.titleA 4.7THz heterodyne receiver for a balloon borne telescopeen_US
dc.typeArticleen_US
dc.identifier.citationHayton, D. J., J. L. Kloosterman, Y. Ren, T. Y. Kao, J. R. Gao, T. M. Klapwijk, Q. Hu, C. K. Walker, and J. L. Reno. “A 4.7THz Heterodyne Receiver for a Balloon Borne Telescope.” Edited by Wayne S. Holland and Jonas Zmuidzinas. Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII (July 23, 2014). © 2014 Society of Photo-Optical Instrumentation Engineers (SPIE)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Electrical Engineering and Computer Scienceen_US
dc.contributor.mitauthorKao, T.-Y.en_US
dc.contributor.mitauthorHu, Qingen_US
dc.relation.journalProceedings of SPIE--the International Society for Optical Engineeringen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dspace.orderedauthorsHayton, D. J.; Kloosterman, J. L.; Ren, Y.; Kao, T. Y.; Gao, J. R.; Klapwijk, T. M.; Hu, Q.; Walker, C. K.; Reno, J. L.en_US
dc.identifier.orcidhttps://orcid.org/0000-0003-1982-4053
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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