Recent science results with the two-telescope IOTA

R. Millan-Gabet; E. Pedretti; J.~D. Monnier; W.~A. Traub; F.~P. Schloerb; N.~P. Carleton; S. Ragland; M.~G. Lacasse; W.~C. Danchi; P.~G. Tuthill; G.~S. Perrin; V. Coudé du Foresto

doi:10.1117/12.459687

Recent science results with the two-telescope IOTA

R. Millan-Gabet, E. Pedretti, J.~D. Monnier, W.~A. Traub, F.~P. Schloerb, N.~P. Carleton, S. Ragland, M.~G. Lacasse, W.~C. Danchi, P.~G. Tuthill, G.~S. Perrin, V. Coudé du Foresto

School of Engineering & Physical Sciences

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

5 Citations (Scopus)

Abstract

The IOTA (Infrared Optical Telescope Array) has been routinely operating with two-telescopes since 1994, a mode destined to become obsolete following its recent conversion to a three-telescope array. In two-telescope mode, the IOTA has made numerous scientific and technical contributions, see e.g. our list of publications at http://cfa-www.harvard.edu/cfa/oir/IOTA/PUBLI/publications.html. We present preliminary results on three different topics using recent data from the two-telescope IOTA: (1) measurements of Mira star diameters simultaneously in three different near-infrared spectral bands, (2) measurement of the characteristic size and shape of the source of near-infared emission in the x-ray binary system CI Cam, and (3) aperture synthesis of the Carbon star V Hydrae combining data from the IOTA and from aperture masking at the Keck-I telescope.

Original language	Undefined/Unknown
Title of host publication	Interferometry for Optical Astronomy II
Editors	W.~A. Traub
Pages	202-209
Number of pages	8
Volume	4838
DOIs	https://doi.org/10.1117/12.459687
Publication status	Published - 24 Feb 2003

Publication series

Name	Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

Access to Document

10.1117/12.459687

Cite this

Millan-Gabet, R., Pedretti, E., Monnier, J. D., Traub, W. A., Schloerb, F. P., Carleton, N. P., Ragland, S., Lacasse, M. G., Danchi, W. C., Tuthill, P. G., Perrin, G. S., & Coudé du Foresto, V. (2003). Recent science results with the two-telescope IOTA. In W. A. Traub (Ed.), Interferometry for Optical Astronomy II (Vol. 4838, pp. 202-209). (Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series). https://doi.org/10.1117/12.459687

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title = "Recent science results with the two-telescope IOTA",

abstract = "The IOTA (Infrared Optical Telescope Array) has been routinely operating with two-telescopes since 1994, a mode destined to become obsolete following its recent conversion to a three-telescope array. In two-telescope mode, the IOTA has made numerous scientific and technical contributions, see e.g. our list of publications at http://cfa-www.harvard.edu/cfa/oir/IOTA/PUBLI/publications.html. We present preliminary results on three different topics using recent data from the two-telescope IOTA: (1) measurements of Mira star diameters simultaneously in three different near-infrared spectral bands, (2) measurement of the characteristic size and shape of the source of near-infared emission in the x-ray binary system CI Cam, and (3) aperture synthesis of the Carbon star V Hydrae combining data from the IOTA and from aperture masking at the Keck-I telescope.",

author = "R. Millan-Gabet and E. Pedretti and J.~D. Monnier and W.~A. Traub and F.~P. Schloerb and N.~P. Carleton and S. Ragland and M.~G. Lacasse and W.~C. Danchi and P.~G. Tuthill and G.~S. Perrin and {Coud{\'e} du Foresto}, V.",

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doi = "10.1117/12.459687",

language = "Undefined/Unknown",

volume = "4838",

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Millan-Gabet, R, Pedretti, E, Monnier, JD, Traub, WA, Schloerb, FP, Carleton, NP, Ragland, S, Lacasse, MG, Danchi, WC, Tuthill, PG, Perrin, GS & Coudé du Foresto, V 2003, Recent science results with the two-telescope IOTA. in WA Traub (ed.), Interferometry for Optical Astronomy II. vol. 4838, Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series, pp. 202-209. https://doi.org/10.1117/12.459687

TY - GEN

T1 - Recent science results with the two-telescope IOTA

AU - Millan-Gabet, R.

AU - Pedretti, E.

AU - Monnier, J.~D.

AU - Traub, W.~A.

AU - Schloerb, F.~P.

AU - Carleton, N.~P.

AU - Ragland, S.

AU - Lacasse, M.~G.

AU - Danchi, W.~C.

AU - Tuthill, P.~G.

AU - Perrin, G.~S.

AU - Coudé du Foresto, V.

PY - 2003/2/24

Y1 - 2003/2/24

N2 - The IOTA (Infrared Optical Telescope Array) has been routinely operating with two-telescopes since 1994, a mode destined to become obsolete following its recent conversion to a three-telescope array. In two-telescope mode, the IOTA has made numerous scientific and technical contributions, see e.g. our list of publications at http://cfa-www.harvard.edu/cfa/oir/IOTA/PUBLI/publications.html. We present preliminary results on three different topics using recent data from the two-telescope IOTA: (1) measurements of Mira star diameters simultaneously in three different near-infrared spectral bands, (2) measurement of the characteristic size and shape of the source of near-infared emission in the x-ray binary system CI Cam, and (3) aperture synthesis of the Carbon star V Hydrae combining data from the IOTA and from aperture masking at the Keck-I telescope.

AB - The IOTA (Infrared Optical Telescope Array) has been routinely operating with two-telescopes since 1994, a mode destined to become obsolete following its recent conversion to a three-telescope array. In two-telescope mode, the IOTA has made numerous scientific and technical contributions, see e.g. our list of publications at http://cfa-www.harvard.edu/cfa/oir/IOTA/PUBLI/publications.html. We present preliminary results on three different topics using recent data from the two-telescope IOTA: (1) measurements of Mira star diameters simultaneously in three different near-infrared spectral bands, (2) measurement of the characteristic size and shape of the source of near-infared emission in the x-ray binary system CI Cam, and (3) aperture synthesis of the Carbon star V Hydrae combining data from the IOTA and from aperture masking at the Keck-I telescope.

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DO - 10.1117/12.459687

M3 - Conference contribution

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T3 - Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series

SP - 202

EP - 209

BT - Interferometry for Optical Astronomy II

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