X- To Ka- Band cryogenic LNA module for very long baseline interferometry

Title X- To Ka- Band cryogenic LNA module for very long baseline interferometry
Author Fung, A., Samoska, L., Bowen, J., Montanez, S., Kooi, J., Soriano, M., Jacobs, C., Manthena, R., Hoppe, D., Akgiray, Ahmed Halid, Lai, R., Mei, X., Barsky, M.
Publication Date: 2020
Publication Place - IEEE
Subject Indium phosphide, HEMT, Low noise, Amplifier, Coaxial module, Cryogenic
Type Document
Language English
Digital Yes
Manuscript No
Library: Özyeğin University
Library Asset ID 978-1-7281-6815-9
Record ID 708d6b7e-1258-4e6e-b24d-eb780fd12467
Library Location Electrical & Electronics Engineering
Date 2020
Sample Text We report a new result of a packaged low noise amplifier (LNA) module with wide bandwidth of 5 to 35 GHz and low noise temperature performance of 10 -18 K, while operated at 10 K ambient. The LNA used 3-stages of sub-50 nm gate length, 100% indium channel content indium phosphide (InP) high electron mobility transistors (HEMTs). Wideband cryogenic LNAs are important for future radio astronomy observatories. To our knowledge these results represent the lowest noise achieved in a wideband amplifier from 5-35 GHz.
DOI 10.1109/IMS30576.2020.9224106
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X- To Ka- Band cryogenic LNA module for very long baseline interferometry

Author Fung, A., Samoska, L., Bowen, J., Montanez, S., Kooi, J., Soriano, M., Jacobs, C., Manthena, R., Hoppe, D., Akgiray, Ahmed Halid, Lai, R., Mei, X., Barsky, M.
Publication Date 2020
Publication Place - IEEE
Subject Indium phosphide, HEMT, Low noise, Amplifier, Coaxial module, Cryogenic
Type Document
Language English
Digital Yes
Manuscript No
Library Özyeğin University
Library Asset ID 978-1-7281-6815-9
Record ID 708d6b7e-1258-4e6e-b24d-eb780fd12467
Library Location Electrical & Electronics Engineering
Date 2020
Sample Text We report a new result of a packaged low noise amplifier (LNA) module with wide bandwidth of 5 to 35 GHz and low noise temperature performance of 10 -18 K, while operated at 10 K ambient. The LNA used 3-stages of sub-50 nm gate length, 100% indium channel content indium phosphide (InP) high electron mobility transistors (HEMTs). Wideband cryogenic LNAs are important for future radio astronomy observatories. To our knowledge these results represent the lowest noise achieved in a wideband amplifier from 5-35 GHz.
DOI 10.1109/IMS30576.2020.9224106
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