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Stellar_flare_hits_HD_189733_b_(artist's_impression)

This artist's impression shows the hot Jupiter HD 189733b, as it passes in front of its parent star, as the latter is flaring, driving material away from the planet. The escaping atmosphere is seen silhouetted against the starlight. The surface of the star, which is around 80% the mass of the Sun, is based on observations of the Sun from NASA's Solar Dynamics Observatory.

Credit: NASA, ESA, L. Calçada, Solar Dynamics Observatory

Prof Suzanne Aigrain

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Exoplanets and planetary physics

Sub department

  • Astrophysics

Research groups

  • Exoplanets and Stellar Physics
Suzanne.Aigrain@physics.ox.ac.uk
Telephone: 01865 (2)73339
Denys Wilkinson Building, room 762
Stars & Planets @ Oxford research group website
  • About
  • Publications

A simple method to estimate radial velocity variations due to stellar activity using photometry

Monthly Notices of the Royal Astronomical Society 419:4 (2012) 3147-3158

Authors:

S Aigrain, F Pont, S Zucker
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Gaussian Processes for Time Series Modelling

Philosophical Transactions of the Royal Society A. Mathematical, Physical and Engineering Sciences (2012)

Authors:

S Roberts, M Osborne, M Ebden, S Reece, N Gibson, S Aigrain
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Probing the Physics of Planets and Stars with Transit Data

NEW HORIZONS IN TIME-DOMAIN ASTRONOMY (2012) 105-105
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Statistics of Stellar Variability from Kepler-I: Revisiting Quarter 1 with an Astrophysically Robust Systematics Correction

Astronomy and Astrophysics 539 (2012) A137

Authors:

A McQuillan, S Aigrain, S Roberts
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Statistics of Stellar Variability in Kepler Data with ARC Systematics Removal

NEW HORIZONS IN TIME-DOMAIN ASTRONOMY (2012) 364-+

Authors:

Amy McQuillan, Suzanne Aigrain, Stephen Roberts
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