activity
20152017
most citedCharacterizing 51 Eri b from 1-5 m: a partly-cloudy exoplanet

130 citations · 418 across the 9 of their papers we have counts for

collaborators

13 papers

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.SR20175 cited

Resolving the H-alpha-emitting Region in the Wind of Eta Carinae

Ya-Lin Wu, Nathan Smith, Laird M. Close +2

The massive evolved star Eta Carinae is the most luminous star in the Milky Way and has the highest steady wind mass-loss rate of any known star. Radiative transfer models of the s…

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…

astro-ph.EP2017130 cited

Characterizing 51 Eri b from 1-5 m: a partly-cloudy exoplanet

Abhijith Rajan, Julien Rameau, Robert J. De Rosa +58

We present spectro-photometry spanning 1-5 m of 51 Eridani b, a 2-10 M planet discovered by the Gemini Planet Imager Exoplanet Survey. In this study, we present new…

astro-ph.EP2017

Evidence that the Directly-Imaged Planet HD 131399 Ab is a Background Star

Eric L. Nielsen, Robert J. De Rosa, Julien Rameau +55

We present evidence that the recently discovered, directly-imaged planet HD 131399 Ab is a background star with non-zero proper motion. From new JHK1L' photometry and spectroscopy…