| dc.contributor.author | Aja Abelán, Beatriz | |
| dc.contributor.author | Seelmann-Eggebert, Matthias | |
| dc.contributor.author | Leuther, Arnulf | |
| dc.contributor.author | Massler, Hermann | |
| dc.contributor.author | Schlechtweg, Michael | |
| dc.contributor.author | Gallego Puyol, Juan Daniel | |
| dc.contributor.author | López Fernández, Isaac | |
| dc.contributor.author | Diez González, María del Carmen | |
| dc.contributor.author | Malo Gómez, Inmaculada | |
| dc.contributor.author | Villa Benito, Enrique | |
| dc.contributor.author | Artal Latorre, Eduardo | |
| dc.contributor.other | Universidad de Cantabria | es_ES |
| dc.date.accessioned | 2025-12-04T16:41:27Z | |
| dc.date.available | 2025-12-04T16:41:27Z | |
| dc.date.issued | 2012 | |
| dc.identifier.isbn | 978-1-4673-1085-7 | |
| dc.identifier.other | TRA2009-0304 | es_ES |
| dc.identifier.uri | https://hdl.handle.net/10902/38423 | |
| dc.description.abstract | MMIC Broadband Low Noise Amplifiers (LNA) for radio astronomy applications with 100 nm GaAs metamorphic High Electron Mobility Transistor (mHEMT) process have been developed. Cryogenic performance of a 4–12 GHz and a 25–34 GHz LNAs is presented. The 4–12 GHz LNA cooled at 15 K exhibits an associated gain of 31.5 dB ± 1.8 dB and average noise temperature of 5.3 K with a low power dissipation of 8 mW. Cooled to 15 K the 25–34 GHz amplifier has demonstrated a flat gain of 24.2 dB ± 0.4 dB with 15.2 K average noise temperature, and a very low power dissipation of 2.8 mW on chip. The mHEMT based LNA MMICs have demonstrated excellent noise characteristics at cryogenic temperatures for their use in radio astronomy applications. | es_ES |
| dc.description.sponsorship | This work has been partially funded by the Ministerio de Ciencia e Innovación (Spain) under research program grant TRA2009-0304. | es_ES |
| dc.format.extent | 3 p. | es_ES |
| dc.language.iso | eng | es_ES |
| dc.publisher | Institute of Electrical and Electronics Engineers, Inc. | es_ES |
| dc.rights | © 2012 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works. | es_ES |
| dc.source | IEEE/MTT-S International Microwave Symposium Digest, Montreal, Quebec, Canada, 2012, 1244-1246 | es_ES |
| dc.subject.other | Cryogenic | es_ES |
| dc.subject.other | Low noise amplifier | es_ES |
| dc.subject.other | MMIC | es_ES |
| dc.subject.other | mHEMT | es_ES |
| dc.title | 4-12 GHz and 25-34 GHz cryogenic MHEMT MMIC low noise amplifiers for radio astronomy | es_ES |
| dc.type | info:eu-repo/semantics/conferenceObject | es_ES |
| dc.relation.publisherVersion | https://doi.org/10.1109/MWSYM.2012.6259592 | es_ES |
| dc.rights.accessRights | openAccess | es_ES |
| dc.relation.projectID | info:eu-repo/grantAgreement/MICINN//TRA2009_0304/ES/Amplificadores de Muy Bajo Ruido de Microondas para Radioastronomia (AMBAR)/ | |
| dc.identifier.DOI | 10.1109/MWSYM.2012.6259592 | |
| dc.type.version | acceptedVersion | es_ES |