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NASA NTRS · 20060043247

Laboratory performance of the Keck interferometer nulling beam combiner

Abstract

Now that regular visibility squared measurements are routinely achieved, mid-infrared nulling is the next observing mode to be implemented on the Keck Interferometer. This mode's main objective is the characterization of exo-zodiacal dust disks around nearby main sequence stars in support of the TPF space mission. Keck Nuller also shares numerious characteristics with an interferometric TPF, and will then serve as a technical precursor for this mission. We report here the results obtained in the laboratory with the KI mid-IR nulling beam combiner, which is based on a dual polarization Modified Mach Zender combiner and dispersion and achromatic nulling through zinc-selenide dielectric plates.

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BibTeXRIS

Mennesson, B., Crawford, S. L., Serabyn, E., Martin, S., Creech-Eakman, M., Hardy, G.. 2003-04-01. Laboratory performance of the Keck interferometer nulling beam combiner. https://ntrs.nasa.gov/citations/20060043247

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