Broadband MMIC LNAs for ALMA Band 2+3 With Noise Temperature Below 28 K

Recent advancements in transistor technology, such as the 35 nm InP HEMT, allow for the development of monolithic microwave integrated circuit (MMIC) low noise amplifiers (LNAs) with performance properties that challenge the hegemony of SIS mixers as leading radio astronomy detectors at frequencies...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	IEEE transactions on microwave theory and techniques 2017-05, Vol.65 (5), p.1589-1597
Hauptverfasser:	Cuadrado-Calle, David, George, Danielle, Fuller, Gary A., Cleary, Kieran, Samoska, Lorene, Kangaslahti, Pekka, Kooi, Jacob W., Soria, Mary, Varonen, Mikko, Lai, Richard, Mei, Xiaobing
Format:	Artikel
Sprache:	eng
Schlagworte:	35 nm InP Ambient temperature Amplifiers Atacama Large Millimeter and Submillimeter Array (ALMA) band 2+3 Broadband cryogenic Cryogenic temperature Cryogenics Detectors Low noise low noise amplifier (LNA) Mixers MMIC (circuits) MMICs monolithic microwave integrated circuit (MMIC) Noise Noise temperature Probes Radio astronomy Radio telescopes Receivers Temperature distribution Transistors W-band WR-10
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!