Paper
28 July 2008 Status of the LBT interferometer
Philip M. Hinz, Teresa Bippert-Plymate, Andy Breuninger, Tom Connors, Brian Duffy, Simone Esposito, William Hoffmann, Jihun Kim, Joe Kraus, Thomas McMahon, Manny Montoya, Richard Nash, Olivier Durney, Elliott Solheid, Andrea Tozzi, Vidhya Vaitheeswaran
Author Affiliations +
Abstract
The Large Binocular Telescope Interferometer, a thermal infrared imager and nulling interferometer for the LBT, is currently being integrated and tested at Steward Observatory. The system consists of a general purpose or universal beamcombiner (UBC) and three camera ports, one of which is populated currently by the Nulling and Imaging Camera (NIC). Wavefront sensing is carried out using pyramid-based "W" units developed at Arcetri Observatory. The system is designed for high spatial resolution, high dynamic range imaging in the thermal infrared. A key project for the program is to survey nearby stars for debris disks down to levels which may obscure detection of Earth-like planets. During 2007-2008 the UBC portion of the LBTI was assembled and tested at Steward Observatory. Initial integration of the system with the LBT is currently in progress as the W units and NIC are being completed in parallel.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Philip M. Hinz, Teresa Bippert-Plymate, Andy Breuninger, Tom Connors, Brian Duffy, Simone Esposito, William Hoffmann, Jihun Kim, Joe Kraus, Thomas McMahon, Manny Montoya, Richard Nash, Olivier Durney, Elliott Solheid, Andrea Tozzi, and Vidhya Vaitheeswaran "Status of the LBT interferometer", Proc. SPIE 7013, Optical and Infrared Interferometry, 701328 (28 July 2008); https://doi.org/10.1117/12.790211
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Cited by 33 scholarly publications.
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KEYWORDS
Mirrors

Interferometers

Telescopes

Cameras

Wavefront sensors

Imaging systems

Infrared radiation

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