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most citedA terrestrial planet candidate in a temperate orbit around Proxima Centauri

1.3k citations · 8.4k across the 150 of their papers we have counts for

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astro-ph.EP2016★ 1.3k cited

A terrestrial planet candidate in a temperate orbit around Proxima Centauri

Guillem Anglada-Escudé, Pedro J. Amado, John Barnes +28

At a distance of 1.295 parsecs, the red-dwarf Proxima Centauri ( Centauri C, GL 551, HIP 70890, or simply Proxima) is the Sun's closest stellar neighbor and one of the best stud…

astro-ph.EP2016★ 119 cited

The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)c

D. P. Bennett, S. H. Rhie, A. Udalski +79

We present the analysis of the first circumbinary planet microlensing event, OGLE-2007-BLG-349. This event has a strong planetary signal that is best fit with a mass ratio of $q \a…

astro-ph.SR2016★ 25 cited

OGLE-2015-BLG-0479LA,B: Binary Gravitational Microlens Characterized by Simultaneous Ground-based and Space-based Observation

C. Han, A. Udalski, A. Gould +60

We present a combined analysis of the observations of the gravitational microlensing event OGLE-2015-BLG-0479 taken both from the ground and by the {\it Spitzer Space Telescope}. T…

astro-ph.EP2016★ 26 cited

First simultaneous microlensing observations by two space telescopes: & reveal a brown dwarf in event OGLE-2015-BLG-1319

Y. Shvartzvald, Z. Li, A. Udalski +90

Simultaneous observations of microlensing events from multiple locations allow for the breaking of degeneracies between the physical properties of the lensing system, specifically…

astro-ph.EP2016★ 17 cited

Discovery of a Gas giant Planet in Microlensing Event OGLE-2014-BLG-1760

A. Bhattacharya, D. P. Bennett, I. A. Bond +41

We present the analysis of the planetary microlensing event OGLE-2014-BLG-1760, which shows a strong light curve signal due to the presence of a Jupiter mass-ratio planet. One unus…

astro-ph.EP2016★ 18 cited

The OGLE-III planet detection efficiency from six years of microlensing observations (2003 to 2008)

Y. Tsapras, M. Hundertmark, Ł. Wyrzykowski +17

We use six years (2003 to 2008) of Optical Gravitational Lensing Experiment III microlensing observations to derive the survey detection efficiency for a range of planetary masses…