24 July 1998 Recent results from the IOTA interferometer
Author Affiliations +
The IOTA interferometer has been in scheduled operation since 1995 with two 0.45 m telescopes, and baselines of up to 38 m; a third telescope will be installed in 1998 and three-beam combination will be implemented in 1999. We currently have three major detection systems, built around a CCD, a NICMOS3, and the FLUOR fiber beam combiner. A piezo- driven rapid scan delay is also available. Our experience in using these systems is reviewed here, and the corresponding magnitude limits of fringe measurements in the V, R, I, J, H, K bands are discussed. Recent result from these new detector systems include measurements of stellar diameters and temperatures, stellar surface features, and circumstellar dust emission.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Wesley A. Traub, "Recent results from the IOTA interferometer", Proc. SPIE 3350, Astronomical Interferometry, (24 July 1998); doi: 10.1117/12.317152; https://doi.org/10.1117/12.317152


Current status of the IOTA interferometer
Proceedings of SPIE (June 09 1994)
Debris collision warning sensor telescope design
Proceedings of SPIE (December 01 1991)
Astronomical Speckle Interferometry In The Infrared
Proceedings of SPIE (November 25 1985)
Assi : An Optimized Fringe Tracking Stellar Interferometer
Proceedings of SPIE (September 20 1989)

Back to Top