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Proceedings Article

IOTA: recent science and technology

[+] Author Affiliations
F. Peter Schloerb, G. Wallace

Univ. of Massachusetts

J.-P. Berger, P. Y. Kern, F. Malbet, K. Rousselet-Perraut

Lab. d'Astrophysique de Grenoble (France)

N. P. Carleton, M. G. Lacasse, M. R. Pearlman, P. A. Schuller

Smithsonian Astrophysical Observatory

P. Hagenauer

Alcatel Space Industries (France)

P. R. Labeye

CEA-LETI (France)

R. Millan-Gabet

California Institute of Technology

J. D. Monnier, E. Pedretti

Univ. of Michigan

S. D. Ragland

California Association for Research in Astronomy

W. A. Traub

Jet Propulsion Lab. and Smithsonian Astrophysical Observatory

Proc. SPIE 6268, Advances in Stellar Interferometry, 62680I (June 27, 2006); doi:10.1117/12.672597
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From Conference Volume 6268

  • Advances in Stellar Interferometry
  • John D. Monnier; Markus Schöller; William C. Danchi
  • Orlando, Florida , USA | May 24, 2006

abstract

We present a brief review of recent scientific and technical advances at the Infrared Optical Telescope Array (IOTA). IOTA is a long-baseline interferometer located atop Mount Hopkins, Arizona. Recent work has emphasized the use of the three-telescope interferometer completed in 2002. We report on results obtained on a range of scientific targets, including AGB stars, Herbig AeBe Stars, binary stars, and the recent outburst of the recurrent nova RS Oph. We report the completion of a new spectrometer which allows visibility measurements at several high spectral resolution channels simultaneously. Finally, it is our sad duty to report that IOTA will be closed this year.

© (2006) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

F. Peter Schloerb ; J.-P. Berger ; N. P. Carleton ; P. Hagenauer ; P. Y. Kern, et al.
"IOTA: recent science and technology", Proc. SPIE 6268, Advances in Stellar Interferometry, 62680I (June 27, 2006); doi:10.1117/12.672597; http://dx.doi.org/10.1117/12.672597


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