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A multi-chroic kinetic inductance detectors array using hierarchical phased array antenna
by
Beyer, Andrew
, Day, Peter K
, Sayers, Jack
, Shu, Shibo
, Golwala, Sunil
, Defrance, Fabien
in
Aluminum
/ Amorphous silicon
/ Antenna arrays
/ Antennas
/ Atmospheric windows
/ Broadband
/ Design
/ Inductance
/ Microstrip transmission lines
/ Niobium
/ Parallel plates
/ Phased arrays
/ Pixels
2022
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A multi-chroic kinetic inductance detectors array using hierarchical phased array antenna
by
Beyer, Andrew
, Day, Peter K
, Sayers, Jack
, Shu, Shibo
, Golwala, Sunil
, Defrance, Fabien
in
Aluminum
/ Amorphous silicon
/ Antenna arrays
/ Antennas
/ Atmospheric windows
/ Broadband
/ Design
/ Inductance
/ Microstrip transmission lines
/ Niobium
/ Parallel plates
/ Phased arrays
/ Pixels
2022
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While trying to remove the title from your shelf something went wrong :( Kindly try again later!
Do you wish to request the book?
A multi-chroic kinetic inductance detectors array using hierarchical phased array antenna
by
Beyer, Andrew
, Day, Peter K
, Sayers, Jack
, Shu, Shibo
, Golwala, Sunil
, Defrance, Fabien
in
Aluminum
/ Amorphous silicon
/ Antenna arrays
/ Antennas
/ Atmospheric windows
/ Broadband
/ Design
/ Inductance
/ Microstrip transmission lines
/ Niobium
/ Parallel plates
/ Phased arrays
/ Pixels
2022
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A multi-chroic kinetic inductance detectors array using hierarchical phased array antenna
Paper
A multi-chroic kinetic inductance detectors array using hierarchical phased array antenna
2022
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Overview
We present a multi-chroic kinetic inductance detector (KID) pixel design integrated with a broadband hierarchical phased-array antenna. Each low-frequency pixel consists of four high-frequency pixels. Four passbands are designed from 125 to 365 GHz according to the atmospheric windows. The lumped element KIDs consist of 100-nm thick AlMn inductors and Nb parallel plate capacitors with hydrogenated amorphous Si dielectric. Two different coupling structures are designed to couple millimeter-wave from microstrip lines to KIDs. The KID designs are optimized for a 10-m-class telescope at a high, dry site, for example, the Leighton Chajnantor Telescope. Preliminary measurement results using Al KIDs are discussed.
Publisher
Cornell University Library, arXiv.org
Subject
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