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Open AccessJournal ArticleDOI

Ground-based coronagraphy with high-order adaptive optics

TLDR
In this article, the authors present simulations of coronagraphs matched to adaptive optics (AO) systems on the Calypso 1.2 m, Palomar Hale 5 m, and Gemini 8 m telescopes under various atmospheric conditions and identify useful parameter ranges for AO coronagraphy.
Abstract
We summarize the theory of coronagraphic optics and identify a dimensionless —ne-tuning parameter, F, which we use to describe the Lyot stop size in the natural units of the coronagraphic optical train and the observing wavelength. We then present simulations of coronagraphs matched to adaptive optics (AO) systems on the Calypso 1.2 m, Palomar Hale 5 m, and Gemini 8 m telescopes under various atmospheric conditions and identify useful parameter ranges for AO coronagraphy on these telescopes. Our simulations employ a tapered, high-pass —lter in spatial frequency space to mimic the action of adaptive wave front correction. We test the validity of this representation of AO correction by comparing our simulations with recent K-band data from the 241 channel Palomar Hale AO system and its dedicated Palomar High Angular Resolution Observer (PHARO) science camera in coronagraphic mode. Our choice of monochromatic modeling enables us to distinguish between underlying halo suppression and ★ b)

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Journal ArticleDOI

First light of the Gemini Planet Imager

TL;DR: Observations ofBeta Pictoris clearly detect the planet, Beta Pictoris b, in a single 60-s exposure with minimal postprocessing, and fitting the Keplerian orbit of Beta Pic b using the new position together with previous astrometry gives a factor of 3 improvement in most parameters over previous solutions.
Journal ArticleDOI

Detection and characterization of exoplanets and disks using projections on karhunen-loève eigenimages

TL;DR: In this paper, a new method to achieve point-spread function (PSF) subtractions for high-contrast imaging using principal component analysis that is applicable to both point sources or extended objects (disks) is described.
Book

The Exoplanet Handbook

TL;DR: In this paper, the authors present an overview of the solar system and its evolution, including the formation and evolution of stars, asteroids, and free-floating planets, as well as their internal and external structures.
Journal ArticleDOI

Detection and Characterization of Exoplanets and Disks using Projections on Karhunen-Loeve Eigenimages

TL;DR: In this article, a new method to achieve point spread function (PSF) subtractions for high contrast imaging using principal component analysis (PCA) that is applicable to both point sources or extended objects (disks) is described.
Journal ArticleDOI

SPHERE: the exoplanet imager for the Very Large Telescope

Jean-Luc Beuzit, +110 more
TL;DR: The Spectro-Polarimetic High contrast imager for Exoplanets REsearch (SPHERE) was designed and built for the ESO Very Large Telescope (VLT) in Chile as mentioned in this paper.
References
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Journal ArticleDOI

Optical Resolution Through a Randomly Inhomogeneous Medium for Very Long and Very Short Exposures

TL;DR: In this article, the average resolution of very-long and very-short-exposure images is studied in terms of the phase and log-amplitude structure functions, whose sum is called the wave-structure function.
Journal ArticleDOI

Discovery of a cool brown dwarf

TL;DR: In this article, the authors reported the discovery of a probable companion to the nearby star G1229, with no more than one-tenth the luminosity of the least luminous hydrogen-burning star.

Discovery of a Cool Brown Dwarf

TL;DR: The discovery of a probable companion to the nearby star G1229, with no more than onetenth the luminosity of the least luminous hydro-gen-burning star, is reported, concluding that the companion is a brown dwarf with a temperature of less than 1,200 K, and a mass ∼20–50 times that of Jupiter.
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