IOTA: recent science and technology

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, G. Wallace

Research output: Contribution to journalArticlepeer-review

4 Citations (Scopus)


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.
Original languageEnglish
Pages (from-to)18
JournalAdvances in Stellar Interferometry
Publication statusPublished - 1 Jul 2006


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