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IOTA: recent science and technology

Schloerb, F. Peter and Berger, J.-P. and Carleton, N. P. and Hagenauer, P. and Kern, P. Y. and Labeye, P. R. and Lacasse, M. G. and Malbet, F. and Millan-Gabet, R. and Monnier, J. D. and Pearlman, M. R. and Pedretti, E. and Rousselet-Perraut, K. and Ragland, S. D. and Schuller, P. A. and Traub, W. A. and Wallace, G. (2006) IOTA: recent science and technology. In: Advances in Stellar Interferometry. Proceedings of SPIE. No.6268. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 62680I. ISBN 9780819463333. https://resolver.caltech.edu/CaltechAUTHORS:20190715-114231327

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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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.672597DOIArticle
ORCID:
AuthorORCID
Berger, J.-P.0000-0001-5025-0428
Lacasse, M. G.0000-0001-8627-9708
Millan-Gabet, R.0000-0003-0447-5866
Monnier, J. D.0000-0002-3380-3307
Additional Information:© 2006 Society of Photo-Optical Instrumentation Engineers (SPIE). The authors gratefully acknowledge the support of the Smithsonian Astrophysical Observatory (for IOTA operation), NASA (for development of the third telescope and NASA NNG05G1180G), the National Science Foundation (AST-0138303, AST-0352723), and the Jet Propulsion Laboratory (JPL Awards 1236050 and 1248252). The IONIC3 instrument has been developed by LAOG and LETI in the context of the IONIC collaboration (LAOG, IMEP, LETI). The IONIC project is funded by the CNRS (France) and the CNES (France). This paper has made use of NASA’s Astrophysics Data System Abstract Service.
Funders:
Funding AgencyGrant Number
Smithsonian Astrophysical ObservatoryUNSPECIFIED
NASANNG05G1180G
NSFAST-0138303
NSFAST-0352723
JPL1236050
JPL1248252
Centre National de la Recherche Scientifique (CNRS)UNSPECIFIED
Centre National d'Études Spatiales (CNES)UNSPECIFIED
Subject Keywords:Infrared, Interferometry, Binary Stars, Mira Stars, Integrated Optics, Closure Phase
Series Name:Proceedings of SPIE
Issue or Number:6268
Record Number:CaltechAUTHORS:20190715-114231327
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190715-114231327
Official Citation:F. Peter Schloerb, J.-P. Berger, N. P. Carleton, P. Hagenauer, P. Y. Kern, P. R. Labeye, M. G. Lacasse, F. Malbet, R. Millan-Gabet, J. D. Monnier, M. R. Pearlman, E. Pedretti, K. Rousselet-Perraut, S. D. Ragland, P. A. Schuller, W. A. Traub, and G. Wallace "IOTA: recent science and technology", Proc. SPIE 6268, Advances in Stellar Interferometry, 62680I (27 June 2006); https://doi.org/10.1117/12.672597
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:97149
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:15 Jul 2019 19:24
Last Modified:14 Oct 2019 19:02

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