activity
20152019
most citedCharacterizing 51 Eri b from 1-5 m: a partly-cloudy exoplanet

130 citations · 322 across the 8 of their papers we have counts for

collaborators

11 papers

astro-ph.EP20193 cited

Directly Imaging Rocky Planets from the Ground

B. Mazin, É. Artigau, V. Bailey +59

Over the past three decades instruments on the ground and in space have discovered thousands of planets outside the solar system. These observations have given rise to an astonishi…

astro-ph.IM201823 cited

Automated data processing architecture for the Gemini Planet Imager Exoplanet Survey

Jason Wang, Marshall Perrin, Dmitry Savransky +49

The Gemini Planet Imager Exoplanet Survey (GPIES) is a multi-year direct imaging survey of 600 stars to discover and characterize young Jovian exoplanets and their environments. We…

astro-ph.IM2017

Precision Time-series Photometry in the Thermal Infrared with a 'Wall-Eyed' Pointing Mode at the Large Binocular Telescope

Eckhart Spalding, Phil Hinz, Andrew Skemer +3

Time-series photometry taken from ground-based facilities is improved with the use of comparison stars due to the short timescales of atmospheric-induced variability. However, the…

astro-ph.SR201725 cited

The TWA 3 Young Triple System: Orbits, Disks, Evolution

Kendra Kellogg, L. Prato, Guillermo Torres +14

We have characterized the spectroscopic orbit of the TWA 3A binary and provide preliminary families of probable solutions for the TWA 3A visual orbit as well as for the wide TWA 3A…

astro-ph.SR201722 cited

The Multiplicity of M-Dwarfs in Young Moving Groups

Yutong Shan, Jennifer C. Yee, Brendan P. Bowler +11

We image 104 newly identified low-mass (mostly M-dwarf) pre-main sequence members of nearby young moving groups with Magellan Adaptive Optics (MagAO) and identify 27 binaries with…

astro-ph.EP2017119 cited

Improving and Assessing Planet Sensitivity of the GPI Exoplanet Survey with a Forward Model Matched Filter

Jean-Baptiste Ruffio, Bruce Macintosh, Jason J. Wang +49

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 subtract…