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20082026
most citedSpin-orbit angle measurements for six southern transiting planets; New insights into the dynamical origins of hot Jupiters

454 citations · 11.2k across the 169 of their papers we have counts for

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Showing 2014Show all

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astro-ph.EP2014★ 2 cited

Three WASP-South transiting exoplanets: WASP-74b, WASP-83b & WASP-89b

Coel Hellier, D. R. Anderson, A. Collier Cameron +16

We report the discovery of three new transiting hot Jupiters by WASP-South together with the TRAPPIST photometer and the Euler/CORALIE spectrograph. WASP-74b orbits a star of V = 9…

astro-ph.EP2014★ 27 cited

The well-aligned orbit of WASP-84b: evidence for disc migration

D. R. Anderson, A. H. M. J. Triaud, O. D. Turner +12

We report the sky-projected orbital obliquity (spin-orbit angle) of WASP-84b, a 0.70- planet in a 8.52-day orbit around a G9V/K0V star, to be . W…

astro-ph.EP2014★ 63 cited

WASP-94 A and B planets: hot-Jupiter cousins in a twin-star system

M. Neveu-VanMalle, D. Queloz, D. R. Anderson +17

We report the discovery of two hot-Jupiter planets, each orbiting one of the stars of a wide binary system. WASP-94A (2MASS 20550794-3408079) is an F8 type star hosting a transitin…

astro-ph.EP2014★ 44 cited

WASP-117b: a 10-day-period Saturn in an eccentric and misaligned orbit

M. Lendl, A. H. M. J. Triaud, D. R. Anderson +17

We report the discovery of WASP-117b, the first planet with a period beyond 10 days found by the WASP survey. The planet has a mass of , a radius o…

astro-ph.SR2014★ 45 cited

Period and amplitude variations in post-common-envelope eclipsing binaries observed with SuperWASP

M. E. Lohr, A. J. Norton, D. R. Anderson +13

Period or amplitude variations in eclipsing binaries may reveal the presence of additional massive bodies in the system, such as circumbinary planets. Here, we have studied twelve…

astro-ph.SR2014★ 66 cited

On the incidence of eclipsing Am binary systems in the SuperWASP survey

B. Smalley, J. Southworth, O. I. Pintado +18

The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analyse…