Barry Smalley
Keele University
448 Papers
6.6K Citations
Barry Smalley is an academic researcher from Keele University. The author has contributed to research in topics: Planet & Stars. The author has an hindex of 72, co-authored 443 publications. Previous affiliations of Barry Smalley include University College London & Max Planck Society.
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Papers
Discovery and characterization of the exoplanets WASP-148b and c : a transiting system with two interacting giant planets
Guillaume Hébrard,Rodrigo F. Díaz,Alexandre C. M. Correia,A. Collier Cameron,Jacques Laskar,Don Pollacco,Jose-Manuel Almenara,David R. Anderson,S. C. C. Barros,Isabelle Boisse,Aldo S. Bonomo,François Bouchy,G. Boué,P. Boumis,D. J. A. Brown,S. Dalal,M. Deleuil,Olivier Demangeon,Amanda P. Doyle,Carole A. Haswell,Coel Hellier,H. P. Osborn,Flavien Kiefer,Ulrich Kolb,K. Lam,A. Lecavelier des Etangs,T. Lopez,M. Martin-Lagarde,Pierre F. L. Maxted,James McCormac,Louise D. Nielsen,Enric Palle,Jorge Prieto-Arranz,Didier Queloz,Alexandre Santerne,Barry Smalley,Oliver Turner,Stéphane Udry,D. Verilhac,Richard G. West,Peter J. Wheatley,P. A. Wilson +41 more
TL;DR: WASP-148b is a hot Jupiter of 0.72 RJup and 0.29 MJup that transits its host with an orbital period of 8.80 days as mentioned in this paper.
The atmospheric parameters of FGK stars using wavelet analysis of CORALIE spectra
TL;DR: In this article, a wavelet decomposition is used to distinguish between noise, continuum trends, and stellar spectral features in the CORALIE spectra of FGK stars, and a subset of wavelet coefficients from the target spectrum are compared to those from a grid of models in a Bayesian framework to determine the posterior probability distributions of the atmospheric parameters.
WASP-31b: a low-density planet transiting a metal-poor, late-F-type dwarf star
David R. Anderson,A. Collier Cameron,Coel Hellier,Monika Lendl,Tim Lister,Pierre F. L. Maxted,Didier Queloz,Barry Smalley,Alexis M. S. Smith,Amaury H. M. J. Triaud,Richard G. West,D. J. A. Brown,Michaël Gillon,Francesco Pepe,Don Pollacco,Damien Ségransan,Rachel Street,Stéphane Udry +17 more
TL;DR: In this article, the authors reported the discovery of the low-density, transiting giant planet WASP-31b, which is in a 3.4-day orbit around a metal-poor, late-F-type, V = 11.7 dwarf star.
Whole Earth Telescope discovery of a strongly distorted quadrupole pulsation in the largest amplitude rapidly oscillating Ap star
Daniel Luke Holdsworth,Daniel Luke Holdsworth,D. W. Kurtz,Hideyuki Saio,Judith L. Provencal,B. Letarte,Ramotholo Sefako,Véronique Petit,Véronique Petit,Barry Smalley,H. Thomsen,C. L. Fletcher +11 more
TL;DR: In this paper, a new analysis of the rapidly oscillating Ap (roAp) star 2MASS J19400781 − 4420093 (J1940) was presented.
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The Infrared Evolution of Sakurai's Object
TL;DR: A cooling, carbon-rich photospheric spectrum was observable from 1996 to 1998 and a strong and broad helium 1.083 $\mu$m P Cygni line developed, signifying the acceleration of an outer envelope of material to speeds as high as 1000 km s$^{-1}$ at the same time the photosphere of the central star remained quiescent as discussed by the authors.
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