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

130 citations · 458 across the 7 of their papers we have counts for

collaborators

9 papers

astro-ph.IM20193 cited

Performance of the Gemini Planet Imager Non-Redundant Mask and spectroscopy of two close-separation binaries HR 2690 and HD 142527

Alexandra Z. Greenbaum, Anthony Cheetham, Anand Sivaramakrishnan +51

The Gemini Planet Imager (GPI) contains a 10-hole non-redundant mask (NRM), enabling interferometric resolution in complement to its coronagraphic capabilities. The NRM operates bo…

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.EP201741 cited

The Taurus Boundary of Stellar/Substellar (TBOSS) Survey II. Disk Masses from ALMA Continuum Observations

K. Ward-Duong, J. Patience, J. Bulger +9

We report 885m ALMA continuum flux densities for 24 Taurus members spanning the stellar/substellar boundary, with spectral types from M4 to M7.75. Of the 24 systems, 22 are dete…

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…