Characterization of exozodiacal dust with the Keck interferometer, VLTI, and SIM

Details Characterization of exozodiacal dust with the Keck interferometer, VLTI, and SIM Characterization of exozodiacal dust with the Keck interferometer, VLTI, and SIM

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998exdu.work..181c&link_type=abstract

Exozodiacal Dust Workshop, p. 181

Astronomy and Astrophysics

Astronomy

Characterization, Infrared Interferometers, Michelson Interferometers, Spaceborne Telescopes, Astronomical Interferometry, Zodiacal Dust, Space Missions, Very Large Array (Vla), Signal Detection, Signal To Noise Ratios

Scientific paper

This overview discusses three interferometers for characterization of
exozodiacal dust: Keck Interferometer, the Very Large Telescope
Interferometer (VLTI), and the Space Interferometry Mission (SIM). The
emphasis will be toward the Keck Interferometer, as exozodiacal dust
characterization is one of its science requirements.

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