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28 August 2014 NIRISS aperture masking interferometry: an overview of science opportunities
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JWST’s Near-Infrared Imager and Slitless Spectrograph (NIRISS) includes an Aperture Masking Interferometry (AMI) mode designed to be used between 2.7μm and 4.8μm. At these wavelengths, it will have the highest angular resolution of any mode on JWST, and, for faint targets, of any existing or planned infrastructure. NIRISS AMI is uniquely suited to detect thermal emission of young massive planets and will permit the characterization of the mid-IR flux of exoplanets discovered by the GPI and SPHERE adaptive optics surveys. It will also directly detect massive planets found by GAIA through astrometric accelerations, providing the first opportunity ever to get both a mass and a flux measurement for non-transiting giant planets. NIRISS AMI will also enable the study of the nuclear environment of AGNs.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Étienne Artigau, Anand Sivaramakrishnan, Alexandra Z. Greenbaum, René Doyon, Paul Goudfrooij, Alex W. Fullerton, David Lafrenière, Kevin Volk, Loïc Albert, André Martel, K. E. Saavik Ford, and Barry L. McKernan "NIRISS aperture masking interferometry: an overview of science opportunities", Proc. SPIE 9143, Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, 914340 (28 August 2014);


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