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Differential Phase Interferometry with the Keck TelescopesWe summarize the Differential Phase (DP) technique as well as the planned implementation at the Keck Interferometer. Multicolor phase measurements are potentially a powerful astrophysical probe - and can allow ground-based direct detection of extrasolar planets. Better than 0.1 mrad phase measurements in the infrared can allow the Keck Interferometer to detect radiation from the so-called hot-Jupiter or 'Roaster' class of planets. At JPL, we are presently developing and testing instrumentation that will enable these extremely sensitive measurements. First on-sky observations are expected to start in mid-2004. In this article we describe DP and other related techniques, provide an outline of the instrument and present results from preliminary laboratory experiments.
Document ID
20080017927
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
Authors
Vasisht, Gautam
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Colavita, M. Mark
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 24, 2013
Publication Date
June 21, 2004
Subject Category
Astrophysics
Meeting Information
Meeting: SPIE Astronomical Telescopes and Instrumentation
Location: Glasgow, Scotland
Country: United Kingdom
Start Date: June 21, 2004
End Date: June 24, 2004
Sponsors: International Society for Optical Engineering
Distribution Limits
Public
Copyright
Other
Keywords
differential phase
infrared detectors
Keck Interferometer
fringe tracking
group-delay tracking
Stellar Interferometer

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