Wide-IF-Band 90-nm CMOS Image-Rejection Subharmonic Radio-Astronomical Array Receiver Design in 75–110 GHz
Author:
Affiliation:
1. Department of Electrical Engineering, National Yang Ming Chiao Tung University, Hsinchu, Taiwan
2. Department of Electrical and Computer Engineering, University of California at Davis, Davis, CA, USA
Funder
Ministry of Science and Technology, Taiwan
U.S. Department of Energy
Publisher
Institute of Electrical and Electronics Engineers (IEEE)
Subject
Electrical and Electronic Engineering,Radiation
Link
https://ieeexplore.ieee.org/ielam/5503871/9874358/9793582-aam.pdf
Reference20 articles.
1. Analysis of wide‐IF‐band 65 nm‐CMOS mixer for 77–110 GHz radio‐astronomical receiver design
2. A 90 nm-CMOS broadband receiver with 10 dB conversion gain and 15 dB noise figure in 80–110 GHz suitable for multi-pixel imaging arrays
3. 110–140-GHz Wide-IF-Band 65-nm CMOS Receiver Design for Fusion Plasma Diagnostics
4. Comparison of cryogenic W band low noise amplifier based on different III-V HEMT foundry process and technologies;valenziano;Proc SPIE,2014
5. Compact monolithic spiral quadrature coupler design
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