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Proceedings Paper

Calibration and imaging algorithms for full-Stokes optical interferometry
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Paper Abstract

Optical interferometry and polarimetry have separately provided new insights into stellar astronomy, especially in the fields of fundamental parameters and atmospheric models. Optical interferometers will eventually add full-Stokes polarization measuring capabilities, thus combining both techniques. In this paper, we: 1) list the observables, calibration quantities, and data acquisition strategies for both limited and full optical interferometric polarimetry (OIP); 2) describe the masking interferometer AMASING and its polarization measuring enhancement called AMASING-POL; 3) show how a radio interferometry imaging package, CASA, can be used for optical interferometry data reduction; and 4) present imaging simulations for Be stars.

Paper Details

Date Published: 12 September 2012
PDF: 10 pages
Proc. SPIE 8445, Optical and Infrared Interferometry III, 84451X (12 September 2012); doi: 10.1117/12.925781
Show Author Affiliations
Nicholas M. Elias, National Radio Astronomy Observatory (United States)
David Mozurkewich, Seabrook Engineering (United States)
Luke M. Schmidt, New Mexico Institute of Mining and Technology (United States)
Colby A. Jurgenson, New Mexico Institute of Mining and Technology (United States)
Stanislav S. Edel, New Mexico Institute of Mining and Technology (United States)
Carol E. Jones, Western Univ. (Canada)
Robert J. Halonen, Western Univ. (Canada)
Henrique R. Schmitt, Computational Physics, Inc. (United States)
Anders M. Jorgensen, New Mexico Institute of Mining and Technology (United States)
Donald J. Hutter, U.S. Naval Observatory (United States)


Published in SPIE Proceedings Vol. 8445:
Optical and Infrared Interferometry III
Françoise Delplancke; Jayadev K. Rajagopal; Fabien Malbet, Editor(s)

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