Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-13T02:13:56.624Z Has data issue: false hasContentIssue false

Probing the Physics of Planets and Stars with Transit Data

Published online by Cambridge University Press:  20 April 2012

Suzanne Aigrain*
Affiliation:
University of Oxford, Department of Physics, Keble Road, Oxford, OX1 3RH, UK email: Suzanne.Aigrain@astro.ox.ac.uk
Rights & Permissions [Opens in a new window]

Summary

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Virtually all exoplanet detection and characterisation methods are based on time-domain data. This invited talk gave an overview of some recent results in the field, highlighting some of the time-series-specific challenges encountered along the way. In particular it focussed on planetary transits: how to detect shallow, rare transits in noisy data, and how to model them with extreme accuracy to extract information about the transiting planet's atmosphere. Space-based transit surveys also constitute an extraordinary goldmine of information on stellar variability, and the talk touched briefly upon some recent statistical work in that field.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012