Cryogenic beam-combiner for very low background 2- to 20-um interferometry on the 22.8-m Large Binocular Telescope

Donald W. McCarthy Jr.; Erin M. Sabatke; Roland J. Sarlot; Philip M. Hinz; James H. Burge

doi:10.1117/12.390267

5 July 2000 Cryogenic beam-combiner for very low background 2- to 20-μm interferometry on the 22.8-m Large Binocular Telescope

Donald W. McCarthy Jr., Erin M. Sabatke, Roland J. Sarlot, Philip M. Hinz, James H. Burge

Author Affiliations +

Proceedings Volume 4006, Interferometry in Optical Astronomy; (2000) https://doi.org/10.1117/12.390267
Event: Astronomical Telescopes and Instrumentation, 2000, Munich, Germany

Abstract

The 22.8 m Large Binocular Telescope Interferometer will be a uniquely powerful tool for imaging and nulling interferometry at thermal infrared wavelengths (2 - 20 micrometers ) because of the LBT's unusual combination of low emissivity, high spatial resolution, broad (u,v)-plane coverage, and high photometric sensitivity. The gregorian adaptive secondary mirrors permit beam combination after only three warm reflections. They also control the relative pathlength, wavefront tip/tilt, and focus of the two telescope beams, thus greatly simplifying the complexity of the beam-combiner. The resulting four-mirror beam-combiner reimages the original focal plane and also images the telescope pupil onto a cold stop to limit thermal background. At first-light in 2004, an all-reflective, cooled beam-combiner can provide a 2 arcmin diameter field for Fizeau-style imaging as well as the low thermal background and achromaticity required for nulling interferometry.

Citation Download Citation

Donald W. McCarthy Jr., Erin M. Sabatke, Roland J. Sarlot, Philip M. Hinz, and James H. Burge "Cryogenic beam-combiner for very low background 2- to 20-μm interferometry on the 22.8-m Large Binocular Telescope", Proc. SPIE 4006, Interferometry in Optical Astronomy, (5 July 2000); https://doi.org/10.1117/12.390267

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