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Paper Abstract

We present the results of differential phase experiments done with data from the Navy Prototype Optical Interferometer (NPOI). We take advantage of the fact that this instrument simultaneously records 16 spectral channels in the wavelength range 550-850nm, for multiple baselines. We discuss the corrections applied to the data, and show the results obtained for Vega and the Be star β Lyrae.

Paper Details

Date Published: 28 June 2006
PDF: 8 pages
Proc. SPIE 6268, Advances in Stellar Interferometry, 62683B (28 June 2006); doi: 10.1117/12.672396
Show Author Affiliations
Henrique R. Schmitt, Naval Research Lab. (United States)
Interferometrics, Inc. (United States)
Thomas A. Pauls, Naval Research Lab. (United States)
Christopher Tycner, U.S. Naval Observatory (United States)
J. Thomas Armstrong, Naval Research Lab. (United States)
James A. Benson, U.S. Naval Observatory (United States)
James H. Clark, Naval Research Lab. (United States)
Robert B. Hindsley, Naval Research Lab. (United States)
Donald J. Hutter, U.S. Naval Observatory (United States)
Deane M. Peterson, Stony Brook Univ. (United States)
Anders M. Jorgensen, Los Alamos National Lab. (United States)
David Mozurkewich, Seabrook Engineering (United States)
G. Charmaine Gilbreath, Naval Research Lab. (United States)
Robert T. Zavala, U.S. Naval Observatory (United States)

Published in SPIE Proceedings Vol. 6268:
Advances in Stellar Interferometry
John D. Monnier; Markus Schöller; William C. Danchi, Editor(s)

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