by David Bennett, Rachel Akeson, Yann Alibert, Jay Anderson, Etienne Bachelet, Jean-Phillipe Beaulieu, Aparna Bhattacharya, Alan Boss, Valerio Bozza, Stephen Bryson, Derek Buzasi, Sebastiano Calchi Novati, Jessie Christiansen, Shawn D. Domagal-goldman, Michael Endl, Benjamin J. Fulton, Calen B. Henderson, B. Scott Gaudi, Samson A. Johnson, Naoki Koshimoto, Michael Meyer, Gijs D. Mulders, Susan Mullally, Ruth Murray-Clay, David Nataf, Eric Nielsen, Henry Ngo, Ilaria Pascucci, Matthew Penny, Peter Plavchan, Radek Poleski, Clement Ranc, Sean N. Raymond, Leslie Rogers, Johannes Sahlmann, Kailash C. Sahu, Joshua Schlieder, Yossi Shvartzvald, Alessandro Sozzetti, Rachel Street, Takahiro Sumi, Daisuke Suzuki, and Neil Zimmerman
Published onMay 31, 2019
Wide-Orbit Exoplanet Demographics
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Abstract
There is currently a gap in our understanding of wide-orbit planets, which must be filled if we are to understand planet formation and exoplanet habitability. We summarize current and planned exoplanet detection programs using a variety of methods: microlensing (including WFIRST), radial velocities, Gaia astrometry, and direct imaging.
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