eBook High Precision Infra-Red Stellar Interferometry download
by Benjamin F. Lane
Author: Benjamin F. Lane
Publisher: Dissertation.Com. (October 15, 2003)
ePub: 1108 kb
Fb2: 1718 kb
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Category: Math Sciences
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High-Precision Infra-Red Stellar Interferometry. The low infrared background and high atmospheric transparency are the principal advantages of Antarctic Plateau sites for astronomy
High-Precision Infra-Red Stellar Interferometry. Cite this publication. The low infrared background and high atmospheric transparency are the principal advantages of Antarctic Plateau sites for astronomy. However, the poor seeing (between 1 and 3 as) negates much of the sensitivity improvements that the Antarctic atmosphere offers, compared to mid-latitude sites such as Mauna Kea or Cerro Paranal.
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In this paper we report the results of a fiber optics beam-combiner at the focus of the IOTA interferometer. In: Paresce F. (eds) Science with the VLT Interferometer. ESO Astrophysics Symposia (European Southern Observatory). Springer, Berlin, Heidelberg.
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High-precision interferometric techniques under development for extrasolar planet detection and characterization (differential phase, nulling and astrometry) all benefit substantially from the slow, low-altitude turbulence, low water vapor content, and low temperature found on the Antarctic plateau.
PHASE-REFERENCED STELLAR INTERFEROMETRY AT THE PALOMAR TESTBED INTERFEROMETER Benjamin F. Lane Division of Geological and Planetary Sciences, 150-21, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125;. and M. Mark Colavita Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109; (for the PTI Collaboration) Received 2002 August 29; accepted 2002 December 3.
Energy Express Engineering and Laboratory Notes. Hsien-kai Hsiao, K. A. Winick, John D. Monnier, and Jean-Philippe Berger, "An infrared integrated optic astronomical beam combiner for stellar interferometry at 3-4 μm," Opt. Express 17, 18489-18500 (2009).