activity
19972016
most citedAngular Differential Imaging: a Powerful High-Contrast Imaging Technique

1k citations · 2.6k across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2016★ 42 cited

A Brown Dwarf Census from the SIMP Survey

Jasmin Robert, Jonathan Gagné, Étienne Artigau +8

We have conducted a near-infrared (NIR) proper motion survey, the Sondage Infrarouge de Mouvement Propre, in order to discover field ultracool dwarfs (UCD) in the solar neighborhoo…

astro-ph.SR2015★ 19 cited

Discovery And Characterization of Wide Binary Systems With a Very Low Mass Component

Frédérique Baron, David Lafrenière, Étienne Artigau +7

We report the discovery of 14 low-mass binary systems containing mid-M to mid-L dwarf companions with separations larger than 250 AU. We also report the independent discovery of 9…

astro-ph.SR2014★ 52 cited

SIMP J2154-1055: A New Low-Gravity L4 Brown Dwarf Candidate Member of the Argus Association

Jonathan Gagné, David Lafrenière, René Doyon +4

We present SIMP J21543454-1055308, a new L4 brown dwarf identified in the Sondage Infrarouge de Mouvement Propre (SIMP) survey that displays signs of low gravity in its near-inf…

astro-ph2008★ 26 cited

CLOUDS search for variability in brown dwarf atmospheres

B. Goldman, M. C. Cushing, M. S. Marley +21

Context: L-type ultra-cool dwarfs and brown dwarfs have cloudy atmospheres that could host weather-like phenomena. The detection of photometric or spectral variability would provid…

astro-ph2007★ 328 cited

The Gemini Deep Planet Survey -- GDPS

David Lafreniere, Rene Doyon, Christian Marois +10

We present the results of the Gemini Deep Planet Survey, a near-infrared adaptive optics search for giant planets and brown dwarfs around nearby young stars. The observations were…

astro-ph2007★ 15 cited

Improving the speckle noise attenuation of simultaneous spectral differential imaging with a focal plane holographic diffuser

David Lafrenière, René Doyon, Daniel Nadeau Étienne Artigau +2

Direct exoplanet detection is limited by speckle noise in the point spread function (PSF) of the central star. This noise can be reduced by subtracting PSF images obtained simultan…