Paper:	Differential phase mode with the Keck Interferometer
Volume:	194, Working on the Fringe: Optical and IR Interferometry from Ground and Space
Page:	89
Authors:	Akeson, R. L.; Swain, M. R.
Abstract:	We will describe the differential phase mode of the Keck Interferometer. The scientific goal of this mode is the direct detection and spectroscopic characterization of hot, Jupiter mass planets. We will describe the effect caused by the relative color difference between the planet and the parent star and the observational technique, which utilizes two-color phase reference interferometry in the near to mid-infrared.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.044 seconds