This report presents results of recent work on the design of a wideband cryogenic low noise amplifier (LNA). The amplifier operates from 200 MHz to 6 GHz with noise temperatures of 2.8 K and 4.5 K at 1.6 GHz and 5.2 GHz respectively. Design, fabrication and cryogenic test results will be described
Radio Astronomers demand for highly sensitive astronomical facility. Their demand is a radio telesco...
We present the results of a development activity for cryogenic Low Noise Amplifiers based on HEMT te...
In this paper, we present the first characterization of GaN-based Low-Noise Amplifiers (LNAs) at cry...
This report presents results of recent work on the design of a wideband cryogenic low noise amplifie...
In investigating star-burst galaxies in the early universe, a radio telescope requires a large inter...
In this letter, the design and measurement of the first SiGe integrated-circuit LNA specifically des...
0.5–13 and 24–40 GHz broadband cryogenic monolithic- microwave integrated-circuit low-noise amplifie...
Four ultra-low noise cryogenic MMIC LNAs suitable for the Square Kilometer Array (SKA) band 2 to 5 (...
In this paper we present the design, modeling, and on-wafer measurement results of an ultra- wideban...
In most radio astronomy instrumentation, cryogenic low noise amplifiers (LNA) are used as intermedia...
MMIC Broadband Low Noise Amplifiers (LNA) for radio astronomy applications with 100 nm GaAs metamorp...
A 0.5-13 GHz cryogenic MMIC low-noise amplifier (LNA) was designed and fabricated using a 130 nm InP...
This paper reports the development of a cryogenic wideband low-noise amplifier based on a 50-nm meta...
The research of the Advanced Radio Instrumentation Group (ARIG) is focused on the design and develop...
Abstract—In this paper a new design of MMIC based LNA is outlined. This design uses a discrete 100-n...
Radio Astronomers demand for highly sensitive astronomical facility. Their demand is a radio telesco...
We present the results of a development activity for cryogenic Low Noise Amplifiers based on HEMT te...
In this paper, we present the first characterization of GaN-based Low-Noise Amplifiers (LNAs) at cry...
This report presents results of recent work on the design of a wideband cryogenic low noise amplifie...
In investigating star-burst galaxies in the early universe, a radio telescope requires a large inter...
In this letter, the design and measurement of the first SiGe integrated-circuit LNA specifically des...
0.5–13 and 24–40 GHz broadband cryogenic monolithic- microwave integrated-circuit low-noise amplifie...
Four ultra-low noise cryogenic MMIC LNAs suitable for the Square Kilometer Array (SKA) band 2 to 5 (...
In this paper we present the design, modeling, and on-wafer measurement results of an ultra- wideban...
In most radio astronomy instrumentation, cryogenic low noise amplifiers (LNA) are used as intermedia...
MMIC Broadband Low Noise Amplifiers (LNA) for radio astronomy applications with 100 nm GaAs metamorp...
A 0.5-13 GHz cryogenic MMIC low-noise amplifier (LNA) was designed and fabricated using a 130 nm InP...
This paper reports the development of a cryogenic wideband low-noise amplifier based on a 50-nm meta...
The research of the Advanced Radio Instrumentation Group (ARIG) is focused on the design and develop...
Abstract—In this paper a new design of MMIC based LNA is outlined. This design uses a discrete 100-n...
Radio Astronomers demand for highly sensitive astronomical facility. Their demand is a radio telesco...
We present the results of a development activity for cryogenic Low Noise Amplifiers based on HEMT te...
In this paper, we present the first characterization of GaN-based Low-Noise Amplifiers (LNAs) at cry...