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Keck interferometer update

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dc.contributor.author Colavita, M. M. en_US
dc.contributor.author Wizinowich, P. L. en_US
dc.date.accessioned 2004-09-17T18:11:09Z
dc.date.available 2004-09-17T18:11:09Z
dc.date.issued 2002-08-22 en_US
dc.identifier.citation Interferometry in Optical Astronomy II (SPIE) en_US
dc.identifier.citation Waikaloa, Hawaii, USA en_US
dc.identifier.clearanceno 02-2104 en_US
dc.identifier.uri http://hdl.handle.net/2014/10022
dc.description.abstract The Keck Interferometer is a NASA-funded joint development between JPL and the W. M. Keck Observatory. The first phase of the project combines the two 10-m Keck Telescopes for high sensitivity near-infrared fringe visibility measurements, nulling interferometry at 10 pm to measure the quantity of exozodiacal emission around nearby stars, and differential-phase measurements to detect hot Jupiters by their direct emission. First fringes with the interferometer were obtained in March 200 1 using the two Kecks with their A 0 systems. Subsequent engineering work been focusedtoward the visibility mode in the areas of improving sensitivity, increasing automation, and adding functionality, in preparation for the high-precision modes. Recently four shared-risk teams were selected by NASA to participate in early science observations, and initial shared-risk science observations have begun. en_US
dc.format.extent 4087777 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Keck interferometer interferometry nulling en_US
dc.title Keck interferometer update en_US


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