Extreme adaptive optics

O Guyon - Annual Review of Astronomy and Astrophysics, 2018 - annualreviews.org
Over the last two decades, several thousand exoplanets have been identified, and their
study has become a high scientific priority. Direct imaging of nearby exoplanets and the …

High-contrast observations in optical and infrared astronomy

BR Oppenheimer, S Hinkley - Annual Review of Astronomy and …, 2009 - annualreviews.org
High-contrast observations in optical and infrared astronomy are defined as any observation
requiring a technique to reveal a celestial object of interest that is in such close angular …

Fundamental limitations of high contrast imaging set by small sample statistics

D Mawet, J Milli, Z Wahhaj, D Pelat… - The Astrophysical …, 2014 - iopscience.iop.org
In this paper, we review the impact of small sample statistics on detection thresholds and
corresponding confidence levels (CLs) in high-contrast imaging at small angles. When …

The Gemini Planet Imager: from science to design to construction

BA Macintosh, JR Graham, DW Palmer… - Adaptive Optics …, 2008 - spiedigitallibrary.org
The Gemini Planet Imager (GPI) is a facility instrument under construction for the 8-m Gemini
South telescope. It combines a 1500 subaperture AO system using a MEMS deformable …

Non-negative matrix factorization: robust extraction of extended structures

B Ren, L Pueyo, GB Zhu, J Debes… - The Astrophysical …, 2018 - iopscience.iop.org
We apply the vectorized non-negative matrix factorization (NMF) method to the post-
processing of the direct imaging data of exoplanetary systems such as circumstellar disks …

Photometric characterization of exoplanets using angular and spectral differential imaging

A Vigan, C Moutou, M Langlois, F Allard… - Monthly Notices of …, 2010 - academic.oup.com
In recent years, there has been intensive research into the direct detection of exoplanets.
Data obtained in the future with high-contrast imaging instruments, optimized for the direct …

Detection and characterization of exoplanets using projections on karhunen–loeve eigenimages: Forward modeling

L Pueyo - The Astrophysical Journal, 2016 - iopscience.iop.org
ABSTRACT A new class of high-contrast image analysis algorithms that empirically fit and
subtract systematic noise has lead to recent discoveries of faint exoplanet/substellar …

Fast computation of Lyot-style coronagraph propagation

R Soummer, L Pueyo, A Sivaramakrishnan… - Optics …, 2007 - opg.optica.org
We present a new method for numerical propagation through Lyot-style coronagraphs using
finite occulting masks. Standard methods for coronagraphic simulations involve Fast Fourier …

A new high contrast imaging program at Palomar observatory

S Hinkley, BR Oppenheimer… - Publications of the …, 2011 - iopscience.iop.org
We describe a new instrument that forms the core of a long-term high contrast imaging
program at the 200 inch (5 m) Hale Telescope at Palomar Observatory. The primary …

Improving and assessing planet sensitivity of the GPI exoplanet survey with a forward model matched filter

JB Ruffio, B Macintosh, JJ Wang, L Pueyo… - The Astrophysical …, 2017 - iopscience.iop.org
We present a new matched-filter algorithm for direct detection of point sources in the
immediate vicinity of bright stars. The stellar point-spread function (PSF) is first subtracted …