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- W1969133039 abstract "The expected stable point spread function, wide field of view, and sensitivity of the NIRCam instrument on the James Webb Space Telescope (JWST) will allow a simple, classical Lyot coronagraph to detect warm Jovian-mass companions orbiting young stars within 150 pc as well as cool Jupiters around the nearest low-mass stars. The coronagraph can also be used to study protostellar and debris disks. At λ = 4.5 μm, where young planets are particularly bright relative to their stars, and at separations beyond ~0.5 arcseconds, the low space background gives JWST significant advantages over ground-based telescopes equipped with adaptive optics. We discuss the scientific capabilities of the NIRCam coronagraph, describe the technical features of the instrument, and present end-to-end simulations of coronagraphic observations of planets and circumstellar disks." @default.
- W1969133039 created "2016-06-24" @default.
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- W1969133039 date "2007-09-13" @default.
- W1969133039 modified "2023-10-01" @default.
- W1969133039 title "Hunting planets and observing disks with the JWST NIRCam coronagraph" @default.
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- W1969133039 doi "https://doi.org/10.1117/12.734873" @default.
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