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20142024
most citedEuclid. I. Overview of the Euclid mission

550 citations · 827 across the 8 of their papers we have counts for

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6 papers · 1 filter

astro-ph.EP2015★ 2 cited

KELT-7b: A hot Jupiter transiting a bright V=8.54 rapidly rotating F-star

Allyson Bieryla, Karen Collins, Thomas G. Beatty +31

We report the discovery of KELT-7b, a transiting hot Jupiter with a mass of MJ, radius of RJ, and an orbital period of $2.7347749 \pm 0.000…

astro-ph.EP2014★ 36 cited

OGLE-2011-BLG-0265Lb: a Jovian Microlensing Planet Orbiting an M Dwarf

J. Skowron, I. -G. Shin, A. Udalski +121

We report the discovery of a Jupiter-mass planet orbiting an M-dwarf star that gave rise to the microlensing event OGLE-2011-BLG-0265. Such a system is very rare among known planet…

astro-ph.EP2014★ 7 cited

NASA ExoPAG Study Analysis Group 11: Preparing for the WFIRST Microlensing Survey

Jennifer C. Yee, Michael Albrow, Richard K. Barry +12

NASA's proposed WFIRST-AFTA mission will discover thousands of exoplanets with separations from the habitable zone out to unbound planets, using the technique of gravitational micr…

astro-ph.EP2014★ 74 cited

High-precision photometry by telescope defocussing. VI. WASP-24, WASP-25 and WASP-26

John Southworth, T. C. Hinse, M. Burgdorf +55

We present time-series photometric observations of thirteen transits in the planetary systems WASP-24, WASP-25 and WASP-26. All three systems have orbital obliquity measurements, W…

astro-ph.EP2014★ 72 cited

Optimal Survey Strategies and Predicted Planet Yields for the Korean Microlensing Telescope Network

Calen B. Henderson, B. Scott Gaudi, Cheongho Han +4

The Korean Microlensing Telescope Network (KMTNet) will consist of three 1.6m telescopes each with a 4 deg^{2} field of view (FoV) and will be dedicated to monitoring the Galactic…

astro-ph.EP2014★ 73 cited

Predictions for Microlensing Planetary Events from Core Accretion Theory

Wei Zhu, Matthew Penny, Shude Mao +2

We conduct the first microlensing simulation in the context of planet formation model. The planet population is taken from the Ida & Lin core accretion model for stars…