Center for Astronomical Adaptive Optics, Steward Observatory, University of Arizona
Center for Astronomical Adaptive Optics, Steward Observatory, University of Arizona Center for Astronomical Adaptive Optics, Steward Observatory, University of Arizona
CAAO Homepage
Steward Observatory Homepage
The University of Arizona Homepage
LBT
MMT
Note: new site! Give us feedback.
LBTI Image
LBTI Team NASA University of Arizona Keck Interferometer Planet Quest LBTO CAAO JPL Navigator NASA Origins Interface Structure NIL/NOMIC UBC NIREST Operations About LBTI

LBTI - Large Binocular Telescope Interferometer

With the advent of large telescopes and progress with associated technology, planets around other stars are now detectable, both in principle and in reality. In order to further this search, Steward Observatory is undertaking the construction of the LBT Inteferometer (LBTI). The NASA-funded project will use the Large Binocular Telescope as a testbed to develop nulling and Fizeau interferometry for this purpose. Nulling interferometry is a technique which cancels the overwhelming glare from a star by interference of light. This allows the detection of nearby planets or dust disks which would otherwise be obscured by the much brighter star. The technique is being studied in preparation for NASA's Terrestrial Planet Finder Misson. The project is currently completing its design phase. In addition to searching for extrasolar planets the instrument will provide for high resolution, wide-field imaging, allowing the LBT to create images with ten times the resolving power of the Hubble Space Telescope.

Recent Publications
Whack-a-speckle: Focal Plane Wavefront Sensing in Theory and Practice with a Deformable Secondary Mirror and 5-micron Camera
../publications/kenworthy_speckle_spie2006.pdf
  Matthew A. Kenworthy, Philip M. Hinz, J. Roger P. Angel, Ari N. Heinze, Suresh Sivanandam
Advances in Adaptive Optics II, edited by Brent L. Ellerbroek, Domenico Bonaccini Calia, Proc. of SPIE Vol. 6272, 62720E-1-62720E-12, 2006.
A visible/infra-red Low Noise, Fast Readout Wavefront Sensor for all-sky Adaptive Optics
../publications/kenworthy_ulnmux_spie2006.pdf
  Matthew A. Kenworthy, Philip M. Hinz, Suresh Sivanandam, Andrew H. Breuninger, Frank Low
High Energy, Optical, and Infrared Detectors for Astronomy II, edited by David A. Dorn, Andrew D. Holland, Proc. of SPIE Vol. 6276, 62760v-1-62760v-10, 2006.
A high-contrast coronagraph for the MMT using phase apodization: design and observations at 5 microns and 2 lambda/D radius
../publications/Codona_SPIE_6269-61.pdf
  J. L. Codona, P. M. Hinz, M. A. Kenworthy, J. R. P. Angel, and N. J. Woolf
Proc. SPIE, Volume 6269, Ground-based and Airborne Instrumentation for Astronomy, 62691N-1-62691N-12, 2006.
High-Resolution Mid-Infrared Imaging of the Asymptotic Giant Branch Star RV Bootis with the Steward Observatory Adaptive Optics System
../publications/58880.web.pdf
  Biller, B. A.; Close, L. M.; Li, A.; Bieging, J. H.; Hoffmann, W. F.; Hinz, P. M.; Miller, D.; Brusa, G.; Lloyd-Hart, M.; Wildi, F.;Potter D., Oppenheimer, B.D.
The Astrophysical Journal, Volume 620, Issue 1, pp. 450-458.
More...