A 350 GHz array of LEKIDs for balloon-borne CMB observations

We present the design, optimization and laboratory characterization of an array of Lumped Element Kinetic Inductance Detectors sensitive in a frequency band centered at 350 GHz. The array consists of 313 feed-horn coupled pixels with resonant frequencies spread over 250 MHz. We present measured yield, quality factor, responsivity, quasiparticle lifetime, noise equivalent power and optical efficiency. The array is a prototype for one of the four frequency bands of OLIMPO, a balloon-borne instrument with a 2.6 m primary mirror proposed for an Antarctic flight to measure the Sunyaev–Zel’dovich effect in clusters of galaxies and their connecting filaments. Similar arrays could also be used with instruments studying the polarization of the cosmic microwave background radiation.

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Publication Details

Journal
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment
Published
2024-09-06
DOI
https://doi.org/10.1016/j.nima.2024.169847
Citations
1
Primary Topic
Superconducting and THz Device Technology
Type
article
Field-Weighted Citation Impact
0.33
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article

A 350 GHz array of LEKIDs for balloon-borne CMB observations

E. S. Battistelli, John A. ZuHone, A. Paiella, Erwin T. Lau et al.
1 citations
Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment
Superconducting and THz Device Technology
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article

A 350 GHz array of LEKIDs for balloon-borne CMB observations

E. S. Battistelli, John A. ZuHone, A. Paiella, Erwin T. Lau, Camille Avestruz, F. Piacentini, Irina Zhuravleva, S. Masi, Shaul Hanany, G. D’Alessandro, A. Coppolecchia, M. De Petris, F. Columbro, Giorgio Pettinari, P. de Bernardis, F. Cacciotti, Esra Bülbül, Jack Sayers, Scott Cray, L. Lamagna, R. Basu Tackur
article en
1 citations

Abstract

We present the design, optimization and laboratory characterization of an array of Lumped Element Kinetic Inductance Detectors sensitive in a frequency band centered at 350 GHz. The array consists of 313 feed-horn coupled pixels with resonant frequencies spread over 250 MHz. We present measured yield, quality factor, responsivity, quasiparticle lifetime, noise equivalent power and optical efficiency. The array is a prototype for one of the four frequency bands of OLIMPO, a balloon-borne instrument with a 2.6 m primary mirror proposed for an Antarctic flight to measure the Sunyaev–Zel’dovich effect in clusters of galaxies and their connecting filaments. Similar arrays could also be used with instruments studying the polarization of the cosmic microwave background radiation.

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated EquipmentVol. 1069
California Institute of Technology (US), University of Minnesota (US), Jet Propulsion Laboratory (US), University of Miami (US), Istituto Nazionale di Fisica Nucleare (IT), University of Michigan (US), University of Chicago (US), Max Planck Institute for Extraterrestrial Physics (DE), Center for Astrophysics Harvard & Smithsonian (US), Istituto di Fotonica e Nanotecnologie (IT), Sapienza University of Rome (IT)
Affordable and clean energy
Openalex Percentile: Top 35%
Superconducting and THz Device Technology
0.33
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