| dc.contributor.author | Hayton, D. J. | |
| dc.contributor.author | Kloosterman, J. L. | |
| dc.contributor.author | Ren, Y. | |
| dc.contributor.author | Gao, J. R. | |
| dc.contributor.author | Klapwijk, T. M. | |
| dc.contributor.author | Hu, Q. | |
| dc.contributor.author | Walker, C. K. | |
| dc.contributor.author | Reno, J. L. | |
| dc.contributor.author | Kao, T.-Y. | |
| dc.contributor.author | Hu, Qing | |
| dc.date.accessioned | 2015-12-18T13:25:37Z | |
| dc.date.available | 2015-12-18T13:25:37Z | |
| dc.date.issued | 2014-07 | |
| dc.identifier.issn | 0277-786X | |
| dc.identifier.uri | http://hdl.handle.net/1721.1/100425 | |
| dc.description.abstract | We 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.sponsorship | United States. National Aeronautics and Space Administration | en_US |
| dc.description.sponsorship | National Science Foundation (U.S.) | en_US |
| dc.language.iso | en_US | |
| dc.publisher | SPIE | en_US |
| dc.relation.isversionof | http://dx.doi.org/10.1117/12.2055790 | en_US |
| dc.rights | Article 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.source | SPIE | en_US |
| dc.title | A 4.7THz heterodyne receiver for a balloon borne telescope | en_US |
| dc.type | Article | en_US |
| dc.identifier.citation | Hayton, 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.department | Massachusetts Institute of Technology. Department of Electrical Engineering and Computer Science | en_US |
| dc.contributor.mitauthor | Kao, T.-Y. | en_US |
| dc.contributor.mitauthor | Hu, Qing | en_US |
| dc.relation.journal | Proceedings of SPIE--the International Society for Optical Engineering | en_US |
| dc.eprint.version | Final published version | en_US |
| dc.type.uri | http://purl.org/eprint/type/ConferencePaper | en_US |
| eprint.status | http://purl.org/eprint/status/NonPeerReviewed | en_US |
| dspace.orderedauthors | Hayton, 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.orcid | https://orcid.org/0000-0003-1982-4053 | |
| mit.license | PUBLISHER_POLICY | en_US |
| mit.metadata.status | Complete | |