Please use this identifier to cite or link to this item: http://archives.univ-biskra.dz/handle/123456789/2322
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dc.contributor.authorZ. Hamaizia-
dc.contributor.authorN. Sengouga-
dc.contributor.authorM. Missous-
dc.contributor.authorM.C.E. Yagoub-
dc.date.accessioned2013-04-16T11:19:49Z-
dc.date.available2013-04-16T11:19:49Z-
dc.date.issued2013-04-16-
dc.identifier.urihttp://archives.univ-biskra.dz/handle/123456789/2322-
dc.description.abstractn this work, we discuss the design of two low noise amplifiers (LNA) based on 1mm gate-length pHEMT InP transistors using two topologies. Designed for radio-astronomy applica-tions, the first is a cascode circuit with a maximum gain of 15dB and noise figure of 0.6dB, while the second is a 2-stage cascaded amplifier with 27 dB gain and 0.63dB noise figure. The two am-plifiers exhibit an input 1-dB compression point of -22dBm and -26dBm respectively, and a third order input intercept point of -10dBm and -5dBm, respectively. Link http://iopscience.iop.org/1748-0221/5/04/P04008/pdf/1748-0221_5_04_P04008.pdfen_US
dc.language.isoenen_US
dc.subjectHEMT amplifiers; Modeling of microwave systems; Analogue electronic circuitsen_US
dc.titleDesign of a wideband low noise amplifier for radio-astronomy applicationsen_US
dc.typeArticleen_US
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