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Neale P. Gibson
Researcher at Trinity College, Dublin
Publications - 149
Citations - 10990
Neale P. Gibson is an academic researcher from Trinity College, Dublin. The author has contributed to research in topics: Exoplanet & Planet. The author has an hindex of 50, co-authored 132 publications receiving 9554 citations. Previous affiliations of Neale P. Gibson include University of St Andrews & University of Oxford.
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Journal ArticleDOI
A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion
David K. Sing,Jonathan J. Fortney,Nikolay Nikolov,Hannah R. Wakeford,Tiffany Kataria,Thomas M. Evans,Suzanne Aigrain,Gilda E. Ballester,Adam Burrows,Drake Deming,Jean-Michel Desert,Neale P. Gibson,Gregory W. Henry,Catherine M. Huitson,Heather Knutson,Alain Lecavelier des Etangs,Frederic Pont,Adam P. Showman,Alfred Vidal-Madjar,Michael H. Williamson,Paul Wilson +20 more
TL;DR: The difference between the planetary radius measured at optical and infrared wavelengths is an effective metric for distinguishing different atmosphere types, so that strong water absorption lines are seen in clear-atmosphere planets and the weakest features are associated with clouds and hazes.
Journal ArticleDOI
Gaussian processes for time-series modelling
Stephen J. Roberts,Michael A. Osborne,Mark Ebden,Steve Reece,Neale P. Gibson,Suzanne Aigrain +5 more
TL;DR: This paper discusses how domain knowledge influences design of the Gaussian process models and provides case examples to highlight the approaches.
Journal ArticleDOI
The prevalence of dust on the exoplanet HD 189733b from Hubble and Spitzer observations
Frederic Pont,David K. Sing,Neale P. Gibson,Neale P. Gibson,Suzanne Aigrain,Gregory W. Henry,Nawal Husnoo +6 more
TL;DR: In this paper, the authors provided a new tabulation of the transmission spectrum across the entire visible and infrared range of the hot Jupiter HD 189733b from UV to infrared using the STIS, ACS and WFC3 instruments.
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Hubble Space Telescope transmission spectroscopy of the exoplanet HD 189733b: high‐altitude atmospheric haze in the optical and near‐ultraviolet with STIS
David K. Sing,Frederic Pont,Suzanne Aigrain,D. Charbonneau,Jean-Michel Desert,Neale P. Gibson,R. L. Gilliland,Wolfgang Hayek,Gregory W. Henry,Heather A. Knutson,A. Lecavelier des Etangs,Tsevi Mazeh,Avi Shporer,Avi Shporer +13 more
TL;DR: In this article, the authors used time series spectra obtained during two transit events to determine the wavelength dependence of the planetary radius and measure the exoplanet's atmospheric transmission spectrum for the first time over this wavelength range.
Journal ArticleDOI
WASP-12b: the hottest transiting extrasolar planet yet discovered
Leslie Hebb,Andrew Collier-Cameron,B. Loeillet,Don Pollacco,Guillaume Hébrard,Rachel Street,François Bouchy,H. C. Stempels,C. Moutou,E. K. Simpson,Stéphane Udry,Yogesh C. Joshi,Richard G. West,I. Skillen,D. M. Wilson,Iain McDonald,Neale P. Gibson,Suzanne Aigrain,David R. Anderson,C. R. Benn,Damian J. Christian,B. Enoch,Carole A. Haswell,Coel Hellier,Keith Horne,Jonathan Irwin,T. A. Lister,Pierre F. L. Maxted,Michel Mayor,Andrew Norton,N. R. Parley,Frederic Pont,D. Queloz,Barry Smalley,Peter J. Wheatley +34 more
TL;DR: The planet has an equilibrium temperature of T eq = 2516 K caused by its very short period orbit around the hot, twelfth magnitude host star and has the largest radius of any transiting planet yet detected.