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NASA NTRS · 20180007558

A Path to High Efficiency Optical Coupling for HIRMES

Abstract

The high-resolution mid-infrared spectrometer (HIRMES) under development for SOFIA (Stratospheric Observatory for Infrared Astronomy) is an instrument operating in the 25-122 μm spectral range with a spectral resolution R= Δ ʎ /ʎ ~100,000 and has two absorber-coupled transition edge sensor (TES) bolometric detector focal planes. We have developed novel NbTiN low stress absorber coatings which have the required optical impedance across the HIRMES operating band. The low intrinsic stress of these coatings allow for a peak-to-valley corrugation amplitude < 5 μm of the 450 nm thick, 1.4 mm x 1.7 mm detector pixels. Furthermore, these coatings have a superconducting transition temperature ~ 10 K, which allows them to simultaneously serve as an absorber in the desired signal band and a rejection filter at long wavelengths. This attribute makes them especially attractive for ultrasensitive absorber-coupled bolometric detector applications, because it helps in controlling the optical loading from out-of band radiation. We also discuss a novel method for integrating a wedged reflective absorber-termination to the detector array.

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BibTeXRIS

Miller, Timothy M., Brown, Ari-David, Costen, Nicholas, Franz, David, Kutyrev, Alexander, Mikula, Vilem, Miller, Kevin H., Moseley, S. Harvey, Oxborrow, Joseph, Rostem, Karwan, Wollack, Edward J.. 2017-07-17. A Path to High Efficiency Optical Coupling for HIRMES. https://ntrs.nasa.gov/citations/20180007558

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