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Wide-Band Two-Stage GaAs LNA for Radio Astronomy

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TLDR
The design, simulation and measurements of wideband two-stage LNAs using commercially available discrete components and targeting Square Kilometre Array (SKA) focalplane-array verification studies show that low wide-band noise figures and power match are achievable by inner-stage component selection and device bias.
Abstract
This paper presents the design, simulation and measurements of wideband two-stage LNAs using commercially available discrete components and targeting Square Kilometre Array (SKA) focalplane-array verification studies. The design optimization was implemented through simulations based on theoretical work that shows that low wide-band noise figures and power match are achievable by inner-stage component selection and device bias. In contrast to the conventional practice of having each stage of a discrete LNA matched to 50Ω, the inner stage was designed with a mismatching capacitor between the two stages. The measured results are presented for 0.7–1.4 GHz and achieve noise figures below 0.4 dB, gain of at least 28 dB, mid-band input return loss of 7 dB, output P1dB of 18.3 dBm, input-referred IP3 of −15.47 dBm, and power consumption of 500mW with a supply voltage of 5V.

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High-Sensitivity Phased Array Receivers for Radio Astronomy

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Wide-band CMOS LowNoiseAmplifier for Applications inRadioAstronomy

TL;DR: A novel variation on a well-known source-degenerated LNA topology is introduced that allows tuning of the power match centre frequency independently from the frequency at which the LNAs noise figure approaches its minimum noise.
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Noise Performance of a Phased-Array Feed With CMOS Low-Noise Amplifiers

TL;DR: The University of Calgary and the National Research Council (NRC) of Canada are developing a low-noise ambient-temperature phased-array demonstrator for possible use in the Square Kilometer Array radio telescope as mentioned in this paper.
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400-to-800-MHz GaAs pHEMT-Based Wideband LNA for Radio-Astronomy Antenna-Array Feed

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References
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Journal ArticleDOI

The Square Kilometre Array

TL;DR: This paper outlines how the scientific challenges are translated into technical challenges, how the application of recent technology offers the potential of affordably meeting these challenges, and how the choices of technology will ultimately be made.
Journal ArticleDOI

Sub-0.2 dB Noise Figure Wideband Room-Temperature CMOS LNA With Non-50 $\Omega$ Signal-Source Impedance

TL;DR: The noise figure of the presented LNA is to the authors' knowledge the lowest noise figure achieved by a power matched wideband CMOS LNA at room temperature.
Journal ArticleDOI

An 8-20-GHz wide-band LNA design and the analysis of its input matching mechanism

TL;DR: In this paper, a wide-band low-noise amplifier (LNA) design with -10 dB input reflection coefficient and 100-K noise temperature over the 8-20 GHz frequency range at room temperature is presented.
Proceedings ArticleDOI

Wide-band CMOS low noise amplifier for applications in radio astronomy

TL;DR: In this article, a CMOS low noise amplifier (LNA) was proposed for a proof-of-concept design of the square kilometer array (SKA) radio telescope, which allows tuning of the power match center frequency independently from the frequency at which the LNAs noise figure approaches its minimum noise.

Wide-band CMOS LowNoiseAmplifier for Applications inRadioAstronomy

TL;DR: A novel variation on a well-known source-degenerated LNA topology is introduced that allows tuning of the power match centre frequency independently from the frequency at which the LNAs noise figure approaches its minimum noise.
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