Hostname: page-component-7c8c6479df-p566r Total loading time: 0 Render date: 2024-03-27T05:29:41.537Z Has data issue: false hasContentIssue false

The Large Binocular Telescope Interferometer & Adaptive Optics System: On-sky Performance and Results

Published online by Cambridge University Press:  06 January 2014

Vanessa Bailey
Affiliation:
Steward Observatory, University of Arizona, 933 N Cherry Ave., Tucson AZ, 85719
Philip Hinz
Affiliation:
Steward Observatory, University of Arizona, 933 N Cherry Ave., Tucson AZ, 85719
Vidhya Vaitheeswaran
Affiliation:
Steward Observatory, University of Arizona, 933 N Cherry Ave., Tucson AZ, 85719
Andrew Skemer
Affiliation:
Steward Observatory, University of Arizona, 933 N Cherry Ave., Tucson AZ, 85719
Denis Defrère
Affiliation:
Steward Observatory, University of Arizona, 933 N Cherry Ave., Tucson AZ, 85719
Timothy Rodigas
Affiliation:
Steward Observatory, University of Arizona, 933 N Cherry Ave., Tucson AZ, 85719
Simone Esposito
Affiliation:
Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I - 50125, FlorenceItaly email: vbailey@as.arizona.edu
Enrico Pinna
Affiliation:
Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I - 50125, FlorenceItaly email: vbailey@as.arizona.edu
Alfio Puglisi
Affiliation:
Istituto Nazionale di Astrofisica, Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I - 50125, FlorenceItaly email: vbailey@as.arizona.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Increasing spatial resolution and contrast capabilities will make possible new direct detections of exoplanets, exozodis, and circumstellar disks. The Large Binocular Telescope Interferometer (LBTI) has been engineered to sit at the combined focus of the Large Binocular Telescope's two 8.4m apertures. Both apertures are equipped with 672-actuator deformable secondary mirrors, the first of the next generation of “extreme” adaptive optics (AO) systems. We present an overview of the LBTI AO instrument suite and detail current on-sky performance.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013 

References

Close, L., et al. 2012, SPIE, 8447, 84470XGoogle Scholar
Esposito, S., et al. 2011, SPIE, 8149, 814902Google Scholar
Lloyd-Hart, M. 2000, PASP, 768, 264Google Scholar
Konopacky, Q., et al. 2013, Science, 339, 1398CrossRefGoogle Scholar
Millan-Gabet, R., et al. 2011, ApJ, 734, 67Google Scholar
Ragazzoni, R. 1996, JModOpt, 43, 289Google Scholar
Lloyd-Hart, M. 2000, PASP, 112, 264CrossRefGoogle Scholar