Keck Interferometer: progress report

2000; SPIE; Volume: 4006; Linguagem: Inglês

10.1117/12.390221

ISSN

1996-756X

Autores

M. M. Colavita, Peter Wizinowich,

Tópico(s)

Astronomy and Astrophysical Research

Resumo

The Keck Interferometer is a NASA-funded joint development between JPL and the W. M. Keck Observatory. The interferometer will combine the two 10-m Keck telescopes with four 1.8-m outrigger telescopes in several observing modes. These include: nulling interferometry at 10 micrometers to measure the quantity of exozodiacal emission around nearby stars; near-infrared differential-phase measurements to detect `hot Jupiters' by their direct emission; narrow-angle astrometry to search for exoplanets by their astrometric signature; and near-infrared imaging to address a variety of imaging science. Active development of the instrument subsystems and associated infrastructure is underway at JPL and CARA.

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