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20042026
most citedSeven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1

1.6k citations · 23.3k across the 403 of their papers we have counts for

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Showing 2016Show all

12 papers · 1 filter

astro-ph.EP2016★ 53 cited

First limits on the occurrence rate of short-period planets orbiting brown dwarfs

Matthias Y. He, Amaury H. M. J. Triaud, Michaël Gillon

Planet formation theories predict a large but still undetected population of short-period terrestrial planets orbiting brown dwarfs. Should specimens of this population be discover…

astro-ph.EP2016★ 1 cited

WASP-86b and WASP-102b: super-dense versus bloated planets

F. Faedi, Y. Gómez Maqueo Chew, D. Pollacco +38

We report the discovery of two transiting planetary systems: a super dense, sub-Jupiter mass planet WASP-86b (\mpl\ = 0.82 0.06 \mj, \rpl\ = 0.63 0.01 \rj), and a bloat…

astro-ph.EP2016★ 26 cited

Discovery of WASP-113b and WASP-114b, two inflated hot-Jupiters with contrasting densities

S. C. C. Barros, D. J. A. Brown, G. Hébrard +37

We present the discovery and characterisation of the exoplanets WASP-113b and WASP-114b by the WASP survey, {\it SOPHIE} and {\it CORALIE}. The planetary nature of the systems was…

astro-ph.EP2016★ 29 cited

WASP-92b, WASP-93b and WASP-118b: Three new transiting close-in giant planets

K. L. Hay, A. Collier-Cameron, A. P. Doyle +36

We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up spectroscopy and ground…

astro-ph.EP2016★ 79 cited

From dense hot Jupiter to low-density Neptune: The discovery of WASP-127b, WASP-136b and WASP-138b

K. W. F. Lam, F. Faedi, D. J. A. Brown +38

We report three newly discovered exoplanets from the SuperWASP survey. WASP-127b is a heavily inflated super-Neptune of mass 0.18 +/- 0.02 M_J and radius 1.37 +/- 0.04 R_J. This is…

astro-ph.EP2016★ 13 cited

Probing TRAPPIST-1-like systems with K2

Brice-Olivier Demory, Didier Queloz, Yann Alibert +2

The search for small planets orbiting late M dwarfs holds the promise of detecting Earth-size planets for which their atmospheres could be characterised within the next decade. The…