20 October 2004 IOTA: recent technology and science
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Closure-phase science and technology are dominant features of the recent activity at IOTA. Our science projects include imaging several spectroscopic binary stars, imaging YSOs including Herbig AeBe stars, detecting asymmetries in a large sample of Mira stars, and measuring water shells around Miras. Many technology projects were pursued in order to make these science observations possible. These include installation of a third-generation integrated-optics 3-beam combiner (IONIC), completion of the real-time control system software, installation of fringe-packet tracking software, use of narrow sub-H band filters, validation of the phase-closure operation, development of CPLD control of the science camera (PICNIC) and star-tracker camera (LLiST), installation of a new star-tracker camera, expansion of the observing facility, and installation of new semi-automated optical alignment tools.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Wesley Arthur Traub, Wesley Arthur Traub, Jean-Philippe Berger, Jean-Philippe Berger, Michael K. Brewer, Michael K. Brewer, Nathaniel P. Carleton, Nathaniel P. Carleton, Pierre Y. Kern, Pierre Y. Kern, Stefan Kraus, Stefan Kraus, Marc G. Lacasse, Marc G. Lacasse, William H. McGonagle, William H. McGonagle, Rafael Millan-Gabet, Rafael Millan-Gabet, John D. Monnier, John D. Monnier, Ettore Pedretti, Ettore Pedretti, Sam Ragland, Sam Ragland, Robert K. Reich, Robert K. Reich, F. Peter Schloerb, F. Peter Schloerb, Peter A. Schuller, Peter A. Schuller, Kamal Souccar, Kamal Souccar, Gary Wallace, Gary Wallace, "IOTA: recent technology and science", Proc. SPIE 5491, New Frontiers in Stellar Interferometry, (20 October 2004); doi: 10.1117/12.550916; https://doi.org/10.1117/12.550916

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