251 citations · 2.8k across the 42 of their papers we have counts for
5 papers · 1 filter
The Homogenous Study of Transiting Systems (HoSTS). II. The influence of the line list on stellar parameters
Amanda P. Doyle, Barry Smalley, Francesca Faedi +2
The use of high resolution, high signal-to-noise stellar spectra is essential in order to determine the most accurate and precise stellar atmospheric parameters via spectroscopy. T…
Detection of Solar-Like Oscillations, Observational Constraints, and Stellar Models for Cyg, the Brightest Star Observed by the {\it Kepler} Mission
J. A. Guzik, G. Houdek, W. J. Chaplin +52
Cygni is an F3 spectral-type main-sequence star with visual magnitude V=4.48. This star was the brightest star observed by the original Kepler spacecraft mission. Short-cadence…
Determining stellar macroturbulence using asteroseismic rotational velocities from Kepler
Amanda P. Doyle, Guy R. Davies, Barry Smalley +2
The Rossiter-McLaughlin effect observed for transiting exoplanets often requires prior knowledge of the stellar projected equatorial rotational velocity. This is usually provided b…
Accurate spectroscopic parameters of WASP planet host stars
Amanda P. Doyle, B. Smalley, P. F. L. Maxted +8
We have made a detailed spectral analysis of eleven Wide Angle Search for Planets (WASP) planet host stars using high signal-to-noise (S/N) HARPS spectra. Our line list was careful…
The EBLM Project I-Physical and orbital parameters, including spin-orbit angles, of two low-mass eclipsing binaries on opposite sides of the Brown Dwarf limit
Amaury H. M. J. Triaud, Leslie Hebb, David R. Anderson +18
This paper introduces a series of papers aiming to study the dozens of low mass eclipsing binaries (EBLM), with F, G, K primaries, that have been discovered in the course of the WA…