Simulation of aperture synthesis with the Large Binocular Telescope

E. Keith Hege, J Roger P Angel, Matt Cheselka, Michael Lloyd-Hart

Research output: Chapter in Book/Report/Conference proceedingConference contribution

10 Citations (Scopus)

Abstract

The large binocular telescope (LBT) will have two 8.4 m apertures spaced 14.4 m from center to center. Adaptive optics will be used to recover deep, long exposure diffraction-limited images in the infrared. The LBT configuration has a diffraction-limited resolution equivalent to a 22.8 m telescope along the center-to-center baseline. Using simulated LBT images and an iterative blind deconvolution algorithm (IBD - Jefferies and Christou, 1993) a sequence of three exposures, at sufficiently different parallactic angles, allows recovery of imagery nearly equivalent to that of the circumscribing 22.8 m circular aperture. To establish a credibility basis for these simulations we have studied the performance of IBD for image constructions of several examples of atmospherically perturbed and partially corrected stellar and galactic data. IBD is robust against influences of real, non-ideal data obtained from large astronomical telescopes, including partial anisoplanicity and Poisson noise from object, sky, and thermal background. For faint objects, which are sky-background and photon-statistics limited, the use of adaptive optics is presumed in these simulations. IBD removes the dilute aperture point spread function effects in the set of parallactic angle-diverse images linearly combined to produce the circumscribed aperture result. Optimal image combination strategy is considered for multi-aperture imaging array configurations.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
Pages144-155
Number of pages12
Volume2566
StatePublished - 1995
EventAdvanced Imaging Technologies and Commercial Applications - San Diego, CA, USA
Duration: Jul 10 1995Jul 12 1995

Other

OtherAdvanced Imaging Technologies and Commercial Applications
CitySan Diego, CA, USA
Period7/10/957/12/95

Fingerprint

Binoculars
Telescopes
apertures
telescopes
synthesis
Adaptive optics
adaptive optics
simulation
sky
Diffraction
faint objects
Optical transfer function
Deconvolution
point spread functions
configurations
diffraction
imagery
Photons
recovery
Statistics

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Condensed Matter Physics

Cite this

Hege, E. K., Angel, J. R. P., Cheselka, M., & Lloyd-Hart, M. (1995). Simulation of aperture synthesis with the Large Binocular Telescope. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 2566, pp. 144-155)

Simulation of aperture synthesis with the Large Binocular Telescope. / Hege, E. Keith; Angel, J Roger P; Cheselka, Matt; Lloyd-Hart, Michael.

Proceedings of SPIE - The International Society for Optical Engineering. Vol. 2566 1995. p. 144-155.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Hege, EK, Angel, JRP, Cheselka, M & Lloyd-Hart, M 1995, Simulation of aperture synthesis with the Large Binocular Telescope. in Proceedings of SPIE - The International Society for Optical Engineering. vol. 2566, pp. 144-155, Advanced Imaging Technologies and Commercial Applications, San Diego, CA, USA, 7/10/95.
Hege EK, Angel JRP, Cheselka M, Lloyd-Hart M. Simulation of aperture synthesis with the Large Binocular Telescope. In Proceedings of SPIE - The International Society for Optical Engineering. Vol. 2566. 1995. p. 144-155
Hege, E. Keith ; Angel, J Roger P ; Cheselka, Matt ; Lloyd-Hart, Michael. / Simulation of aperture synthesis with the Large Binocular Telescope. Proceedings of SPIE - The International Society for Optical Engineering. Vol. 2566 1995. pp. 144-155
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