Optical characterization of aluminum-based 280 GHz CCAT MKID pixels and arrays

We present the first full-array optical characterizations of the 280 GHz aluminum-based superconducting microwave kinetic inductance detector (MKID) arrays developed at NIST, CO, USA for the CCAT Collaboration for observing galactic ecology, Sunyaev-Zel'dovich effect, galaxy evolution, and line intensity mapping. The main advantage of aluminum MKIDs is their lower 1/f noise compared to the alternative choice of titanium-nitride (TiN) MKIDs, which would reduce systematic drifts when mapping the sky. We will present the spectral response, polarization characteristics, detector efficiency, and noise equivalent power (NEP) under the relevant conditions for these detectors. Two aluminum and one TiN MKID arrays will form the detector arrays in the 280 GHz instrument module of the Prime-Cam. First light observations are expected in 2025.

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Published
2024-08-16
DOI
https://doi.org/10.1117/12.3017858
Primary Topic
Superconducting and THz Device Technology
Type
article
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article

Optical characterization of aluminum-based 280 GHz CCAT MKID pixels and arrays

Adrian K. Sinclair, Alicia Middleton, D. Scott, Rodrigo Freundt et al.
Superconducting and THz Device Technology
article

Optical characterization of aluminum-based 280 GHz CCAT MKID pixels and arrays

Adrian K. Sinclair, Alicia Middleton, D. Scott, Rodrigo Freundt, Thomas Nikola, Jason E. Austermann, Cody J. Duell, James Burgoyne, Michael D. Niemack, James A. Beall, G. J. Stacey, Anthony I. Huber, Samantha Walker, A. T. Crites, Joel N. Ullom, Steve K. Choi, Bugao Zou, Michael Vissers, Zachary B. Huber, Victoria Butler, Jordan Wheeler, Anna Vaskuri, Johannes Hubmayr, Ema Smith, Scott C. Chapman, Jeffrey van Lanen, Eve M. Vavagiakis, Lawrence Lin
article en

Abstract

We present the first full-array optical characterizations of the 280 GHz aluminum-based superconducting microwave kinetic inductance detector (MKID) arrays developed at NIST, CO, USA for the CCAT Collaboration for observing galactic ecology, Sunyaev-Zel'dovich effect, galaxy evolution, and line intensity mapping. The main advantage of aluminum MKIDs is their lower 1/f noise compared to the alternative choice of titanium-nitride (TiN) MKIDs, which would reduce systematic drifts when mapping the sky. We will present the spectral response, polarization characteristics, detector efficiency, and noise equivalent power (NEP) under the relevant conditions for these detectors. Two aluminum and one TiN MKID arrays will form the detector arrays in the 280 GHz instrument module of the Prime-Cam. First light observations are expected in 2025.

University of California, Riverside (US), National Institute of Standards and Technology (US), University of British Columbia (CA), Cornell University (US), University of Victoria (CA)
Affordable and clean energy
Openalex Percentile: Top 89%
Superconducting and THz Device Technology
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