On the Design and Performance of Very Large MKID Arrays [VIDEO]

S.J.C. Yates; J. Bueno; A. Endo; A.M. Baryshev; L. Ferrari; V. Murugesan; D.J. Thoen; J.J.A. Baselmans

doi:10.1117/12.2562367

On the Design and Performance of Very Large MKID Arrays [VIDEO]

S.J.C. Yates, J. Bueno, A. Endo, A.M. Baryshev, L. Ferrari, V. Murugesan, D.J. Thoen, J.J.A. Baselmans

Tera-Hertz Sensing

Research output: Contribution to conference › Other › Other research output

Abstract

Far infra-red, mm and sub-mm astronomy requires very large arrays of detectors for future wide field cameras and spectrometers. We present an array of lens-antenna coupled Microwave Kinetic Inductance Detectors (MKID) for a wide field camera at 350 GHz. We discuss the optimization to maximize the usable detector yield and matching the array to the readout to enable array performance close to the background limit. We overview the optical characterization techniques required to have confidence in the instrument performance prior to on telescope integration, finally giving measured optical performance for an optimized array.

Original language	English
Number of pages	1
DOIs	https://doi.org/10.1117/12.2562367
Publication status	Published - 2020
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X - Virtual/online event due to COVID-19 Duration: 14 Dec 2020 → 18 Dec 2020

Conference

Conference	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X
Abbreviated title	Spie 11453
Period	14/12/20 → 18/12/20

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title = "On the Design and Performance of Very Large MKID Arrays [VIDEO]",

abstract = "Far infra-red, mm and sub-mm astronomy requires very large arrays of detectors for future wide field cameras and spectrometers. We present an array of lens-antenna coupled Microwave Kinetic Inductance Detectors (MKID) for a wide field camera at 350 GHz. We discuss the optimization to maximize the usable detector yield and matching the array to the readout to enable array performance close to the background limit. We overview the optical characterization techniques required to have confidence in the instrument performance prior to on telescope integration, finally giving measured optical performance for an optimized array.",

author = "S.J.C. Yates and J. Bueno and A. Endo and A.M. Baryshev and L. Ferrari and V. Murugesan and D.J. Thoen and J.J.A. Baselmans",

year = "2020",

doi = "10.1117/12.2562367",

language = "English",

note = "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, Spie 11453 ; Conference date: 14-12-2020 Through 18-12-2020",

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TY - CONF

T1 - On the Design and Performance of Very Large MKID Arrays [VIDEO]

AU - Yates, S.J.C.

AU - Bueno, J.

AU - Endo, A.

AU - Baryshev, A.M.

AU - Ferrari, L.

AU - Murugesan, V.

AU - Thoen, D.J.

AU - Baselmans, J.J.A.

PY - 2020

Y1 - 2020

N2 - Far infra-red, mm and sub-mm astronomy requires very large arrays of detectors for future wide field cameras and spectrometers. We present an array of lens-antenna coupled Microwave Kinetic Inductance Detectors (MKID) for a wide field camera at 350 GHz. We discuss the optimization to maximize the usable detector yield and matching the array to the readout to enable array performance close to the background limit. We overview the optical characterization techniques required to have confidence in the instrument performance prior to on telescope integration, finally giving measured optical performance for an optimized array.

AB - Far infra-red, mm and sub-mm astronomy requires very large arrays of detectors for future wide field cameras and spectrometers. We present an array of lens-antenna coupled Microwave Kinetic Inductance Detectors (MKID) for a wide field camera at 350 GHz. We discuss the optimization to maximize the usable detector yield and matching the array to the readout to enable array performance close to the background limit. We overview the optical characterization techniques required to have confidence in the instrument performance prior to on telescope integration, finally giving measured optical performance for an optimized array.

U2 - 10.1117/12.2562367

DO - 10.1117/12.2562367

M3 - Other

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X

Y2 - 14 December 2020 through 18 December 2020

ER -

On the Design and Performance of Very Large MKID Arrays [VIDEO]

Abstract

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