Please use this identifier to cite or link to this item: http://archives.univ-biskra.dz/handle/123456789/2317
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dc.contributor.authorZ. Hamaizia-
dc.contributor.authorN. Sengouga-
dc.contributor.authorM. Missous-
dc.contributor.authorM.C.E. Yagoub-
dc.date.accessioned2013-04-16T10:54:18Z-
dc.date.available2013-04-16T10:54:18Z-
dc.date.issued2013-04-16-
dc.identifier.urihttp://archives.univ-biskra.dz/handle/123456789/2317-
dc.description.abstractIn this work, the design of a novel low-noise amplifier (LNA) based on 1 μm gate-length InGaAs/InAlAs/InP pHEMT transistors is discussed. Designed for radioastronomy applications, this amplifier exploits a common-drain configuration as input stage and a common-source inductive degeneration topology as output stage. It exhibits a maximum gain of 30 dB within an input 1 dB compression point of −16 dBm. The noise figure is 0.4 dB with an input return loss greater than −10 dB and an output return loss of −12.5 dB. The LNA consumes 85 mW from a 1.5 V power supply. Link http://www.sciencedirect.com/science/article/pii/S1369800110000934en_US
dc.language.isoenen_US
dc.subjectHEMT; LNA; SKA; SKADS; Telescope.en_US
dc.titleA 0.4 dB noise figure wideband low-noise amplifier using a novel InGaAs/InAlAs/InP deviceen_US
dc.typeArticleen_US
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