Fizeau Interferometry with the LBT Astronomy on the Way to ELTs

Gaessler, W.; Herbst, T. M.; Ragazzoni, R.; Eckart, A.; Weigelt, G.

Exploring the Cosmic Frontier, ESO Astrophysics Symposia European Southern Observatory, Volume . ISBN 978-3-540-39755-7. Springer, p. 55 (2007)


Abstract
The Large Binocular Telescope (LBT) consists of two 8.4 m mirrors on one mechanical mounting, with a center to center separation of 14.4 m. In the combined, focus the LBT provides the spatial resolution of a 23 m telescope and the sensitivity of a 12 m telescope. We are building an instrument called LINC-NIRVANA using the capability of LBT in Fizeau mode (imaging interferometry), leading to a unique combination of spatial resolution, sensitivity and field of view. The instrument will prove technology, such as Multi-Conjugated Adaptive Optics, which is needed for the next generation of Extremely Large Telescopes (ELT) (20 to 100 m diameter). The capabilities of LINC-NIRVANA will extend science, especially for extragalactic programs, building a bridge between current 10 m class telescopes and ELTs.

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