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20042026
most citedMicrolens OGLE-2005-BLG-169 Implies Cool Neptune-Like Planets are Common

336 citations · 5.3k across the 142 of their papers we have counts for

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Showing 2014Show all

8 papers · 1 filter

astro-ph.SR2014★ 29 cited

Searching for variable stars in the cores of five metal rich globular clusters using EMCCD observations

Jesper Skottfelt, D. M. Bramich, R. Figuera Jaimes +31

In this paper, we present the analysis of time-series observations from 2013 and 2014 of five metal rich ([Fe/H] -1) globular clusters: NGC~6388, NGC~6441, NGC~6528, NGC~6638,…

astro-ph.EP2014★ 299 cited

A ring system detected around the Centaur (10199) Chariklo

F. Braga-Ribas, B. Sicardy, J. L. Ortiz +61

Until now, rings have been detected in the Solar System exclusively around the four giant planets. Here we report the discovery of the first minor-body ring system around the Centa…

astro-ph.EP2014★ 15 cited

Search for the Return of Activity in Active Asteroid 176P/LINEAR

Henry H. Hsieh, Larry Denneau, Alan Fitzsimmons +18

We present the results of a search for the reactivation of active asteroid 176P/LINEAR during its 2011 perihelion passage using deep optical observations obtained before, during, a…

astro-ph.EP2014★ 38 cited

Physical properties of the WASP-67 planetary system from multi-colour photometry

L. Mancini, J. Southworth, S. Ciceri +29

The extrasolar planet WASP-67 b is the first hot Jupiter definitively known to undergo only partial eclipses. The lack of the second and third contact point in this planetary syste…

astro-ph.SR2014★ 19 cited

Candidate Gravitational Microlensing Events for Future Direct Lens Imaging

C. B. Henderson, H. Park, T. Sumi +76

The mass of the lenses giving rise to Galactic microlensing events can be constrained by measuring the relative lens-source proper motion and lens flux. The flux of the lens can be…

astro-ph.EP2014★ 20 cited

MOA-2013-BLG-220Lb: Massive Planetary Companion to Galactic-Disk Host

J. C. Yee, C. Han, A. Gould +70

We report the discovery of MOA-2013-BLG-220Lb, which has a super-Jupiter mass ratio relative to its host. The proper motion, $μ=12.5\pm 1\, {\rm mas}…