activity
20172021
most citedThe Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s

178 citations · 299 across the 11 of their papers we have counts for

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Showing astro-ph.EPShow all

9 papers · 1 filter

astro-ph.EP2021

OGLE-2019-BLG-0960Lb: The Smallest Microlensing Planet

Jennifer C. Yee, Weicheng Zang, Andrzej Udalski +80

We report the analysis of OGLE-2019-BLG-0960, which contains the smallest mass-ratio microlensing planet found to date (q = 1.2--1.6 x 10^{-5} at 1-sigma). Although there is substa…

astro-ph.EP20209 cited

Revealing Short-period Exoplanets and Brown Dwarfs in the Galactic Bulge using the Microlensing Xallarap Effect with the \textit{Nancy Grace Roman Space Telescope}

Shota Miyazaki, Samson A. Johnson, Takahiro Sumi +3

The \textit{Nancy Grace Roman Space Telescope} (\textit{ Roman}) will provide an enormous number of microlensing light curves with much better photometric precisions than ongoing g…

astro-ph.EP2020

The HD 217107 Planetary System: Twenty Years of Radial Velocity Measurements

Mark R. Giovinazzi, Cullen H. Blake, Jason D. Eastman +13

The hot Jupiter HD 217107 b was one of the first exoplanets detected using the radial velocity (RV) method, originally reported in the literature in 1999. Today, precise RV measure…

astro-ph.EP20191 cited

The Scientific Context of WFIRST Microlensing in the 2020s

Jennifer Yee, Rachel Akeson, Jay Anderson +23

[abridged] WFIRST is uniquely capable of finding planets with masses as small as Mars at separations comparable to Jupiter, i.e., beyond the current ice lines of their stars. These…

astro-ph.EP2019

Wide-Orbit Exoplanet Demographics

David P. Bennett, Rachel Akeson, Yann Alibert +41

The Kepler, K2 and TESS transit surveys are revolutionizing our understanding of planets orbiting close to their host stars and our understanding of exoplanet systems in general, b…

astro-ph.EP2019

Masses and Distances of Planetary Microlens Systems with High Angular Resolution Imaging

Aparna Bhattacharya, Rachel Akeson, Jay Anderson +33

Microlensing is the only method that can detect and measure mass of wide orbit, low mass, solar system analog exoplanets. Mass measurements of such planets would yield massive scie…