Journal
MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VI
Volume 8452, Issue -, Pages -Publisher
SPIE-INT SOC OPTICAL ENGINEERING
DOI: 10.1117/12.925759
Keywords
lumped-element; superconductivity; kinetic-inductance; far-infrared; titanium nitride
Funding
- National Aeronautics and Space Administration
- Keck Institute for Space Science
- Gordon and Betty Moore Foundation
- NASA [NNX10AC83]
- Keck Institute for Space Studies
- NASA Postdoctoral Program
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Future submillimeter telescopes will demand arrays with similar to 10(6) pixels to fill the focal plane. MAKO is a 350 mu m camera being developed to demonstrate the use of superconducting microresonators to meet the high multiplexing factors required for scaling to large-format arrays while offering background-limited single-pixel sensitivity. Candidate pixel designs must simultaneously meet many requirements. To achieve the desired noise equivalent powers it must efficiently absorb radiation, feature a high responsivity, and exhibit low intrinsic device noise. Additionally, the use of high resonator quality factors of order similar to 10(5) and resonant frequencies of order f(res) approximate to 100 MHz are desirable in order to reduce the per-pixel bandwidth to a minimum set by telescope scan speeds. This allows a maximum number of pixels to be multiplexed in a fixed electronic bandwidth. Here we present measurement results of the first MAKO prototype array which meets these design requirements while demonstrating sufficient sensitivity for background-limited operation at ground-based, far-infrared telescopes.
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