activity
20152026
most citedKeck/NIRC2 '-Band Imaging of Jovian-Mass Accreting Protoplanets around PDS 70

84 citations · 252 across the 18 of their papers we have counts for

collaborators
Showing 2018Show all

9 papers · 1 filter

astro-ph.EP2018

Detecting Water In the atmosphere of HR 8799 c with L-band High Dispersion Spectroscopy Aided By Adaptive Optics

Ji Wang, Dimitri Mawet, Jonathan J. Fortney +3

High dispersion spectroscopy of brown dwarfs and exoplanets enables exciting science cases, e.g., mapping surface inhomogeneity and measuring spin rate. Here, we present band o…

astro-ph.EP2018

Deep exploration of Eridani with Keck Ms-band vortex coronagraphy and radial velocities: mass and orbital parameters of the giant exoplanet

Dimitri Mawet, Lea Hirsch, Eve J. Lee +27

We present the most sensitive direct imaging and radial velocity (RV) exploration of Eridani to date. Eridani is an adolescent planetary system, reminiscent of the early So…

astro-ph.IM2018

Efficient spectroscopy of exoplanets at small angular separations with vortex fiber nulling

Garreth Ruane, Ji Wang, Dimitri Mawet +4

Instrumentation designed to characterize potentially habitable planets may combine adaptive optics and high-resolution spectroscopy techniques to achieve the highest possible sensi…

astro-ph.SR2018

EPIC 203868608: A low-mass quadruple star system in the Upper Scorpius OB association

Ji Wang, Trevor J. David, Lynne Hillenbrand +3

Young multiple star systems provide excellent testing grounds for theories of star formation and evolution. EPIC 203868608 was previously studied~\citep{David2016} as a triple star…

astro-ph.IM2018

Direct Imaging in Reflected Light: Characterization of Older, Temperate Exoplanets With 30-m Telescopes

Etienne Artigau, Rebecca A. Bernstein, Timothy Brandt +22

Direct detection, also known as direct imaging, is a method for discovering and characterizing the atmospheres of planets at intermediate and wide separations. It is the only means…

astro-ph.IM2018

The Planetary Systems Imager: 2-5 Micron Channel

Andrew J. Skemer, Deno Stelter, Dimitri Mawet +15

We summarize the red channel (2-5 micron) of the Planetary Systems Imager (PSI), a proposed second-generation instrument for the TMT. Cold exoplanets emit the majority of their lig…