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arXiv · 1512.00053

Toward Direct Imaging of Low-Mass Gas-Giants with the $\textit{James Webb Space Telescope}$

Joshua E. Schlieder·Charles A. Beichman·Michael R. Meyer·Thomas Greene
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Abstract

In preparation for observations with the $\textit{James Webb Space Telescope}$ ($\textit{JWST}$), we have identified new members of the nearby, young M dwarf sample and compiled an up to date list of these stars. Here we summarize our efforts to identify young M dwarfs, describe the current sample, and detail its demographics in the context of direct planet imaging. We also describe our investigations of the unprecedented sensitivity of the $\textit{JWST}$ when imaging nearby, young M dwarfs. The $\textit{JWST}$ is the only near term facility capable of routinely pushing direct imaging capabilities around M dwarfs to sub-Jovian masses and will provide key insight into questions regarding low-mass gas-giant properties, frequency, formation, and architectures.

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Joshua E. Schlieder, Charles A. Beichman, Michael R. Meyer, Thomas Greene. 2015-10-13. Toward Direct Imaging of Low-Mass Gas-Giants with the $\textit{James Webb Space Telescope}$. https://arxiv.org/abs/1512.00053

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