output
19922026
most citedThe SIESTA method for ab initio order-N materials simulation

12k citations

Showing 2013 · astro-ph.EPShow all

31 papers · 2 filters

astro-ph.EP2013★ 128 cited

Kepler-91b: a planet at the end of its life. Planet and giant host star properties via light-curve variations

J. Lillo-Box, D. Barrado, A. Moya +8

The evolution of planetary systems is intimately linked to the evolution of their host star. Our understanding of the whole planetary evolution process is based on the large planet…

astro-ph.EP2013

Transiting planets from WASP-South, Euler and TRAPPIST: WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars

L. Delrez, V. Van Grootel, D. R. Anderson +19

We report the discovery by the WASP transit survey of three new hot Jupiters, WASP-68 b, WASP-73 b and WASP-88 b. WASP-68 b has a mass of 0.95+-0.03 M_Jup, a radius of 1.24-0.06+0.…

astro-ph.EP2013★ 55 cited

Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry

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

WASP-80 is one of only two systems known to contain a hot Jupiter which transits its M-dwarf host star. We present eight light curves of one transit event, obtained simultaneously…

astro-ph.EP2013★ 137 cited

Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b

Coel Hellier, D. R. Anderson, A. Collier Cameron +15

We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the ran…

astro-ph.EP2013★ 133 cited

Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b & WASP-90b

R. G. West, J. -M. Almenara, D. R. Anderson +22

We report three new transiting hot-Jupiter planets discovered from the WASP surveys combined with radial velocities from OHP/SOPHIE and Euler/CORALIE and photometry from Euler and…

astro-ph.EP2013★ 318 cited

Stellar Spin-Orbit Misalignment in a Multiplanet System

Daniel Huber, Joshua A. Carter, Mauro Barbieri +32

Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple co-planar planets have been seen to have low obliquities. This has been interpre…