Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-19T07:18:05.070Z Has data issue: false hasContentIssue false
  • English
  • Français

A visual guide to planetary microlensing

Published online by Cambridge University Press:  10 November 2011

Leslie A. Rogers  and
Paul L. Schechter
Leslie A. Rogers
Affiliation:
Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA email: [email protected], [email protected]
Paul L. Schechter
Affiliation:
Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139, USA email: [email protected], [email protected]
Rights & Permissions [Opens in a new window]

Abstract

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.

The microlensing technique has found 10 exoplanets to date and promises to discover more in the near future. While planetary transit light curves all show a familiar shape, planetary perturbations to microlensing light curves can manifest a wide variety of morphologies. We present a graphical guide that may be useful when understanding microlensing events showing planetary caustic perturbations.

Keywords

gravitational lensingplanetary systems
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S276: The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution , October 2010 , pp. 457 - 458
Copyright
Copyright © International Astronomical Union 2011

References

Bennett, D. P. 2008, in: Mason, J. (ed.), Exoplanets (Berlin: Springer), p. 47CrossRefGoogle Scholar
Gaudi, B. S. 2010, in: Seager, S. (ed.), Exoplanets (Tucson, AZ: University of Arizona Press)Google Scholar