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Direct Imaging as a Detection Technique for Exoplanets

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Abstract

In this chapter we review the essential ingredients of exoplanet detection with the direct imaging method. In the first section, we discuss the various sources of noise associated with direct exoplanet detection along with the trades in instrument design that help reduce them. We derive scaling laws from first principles to outline the broad strokes of the compromises that can be made at the instrument level. In the second section we tackle the detection problem from a data analysis standpoint. We present the most widespread class of algorithms and discuss future improvements.

Keywords

  • Exoplanet Detection
  • Coronagraph
  • Host Star
  • Gemini Planet Imager
  • Wavefront Control

These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Correspondence to Laurent Pueyo .

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© 2018 Springer International Publishing AG, part of Springer Nature

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Pueyo, L. (2018). Direct Imaging as a Detection Technique for Exoplanets. In: Deeg, H., Belmonte, J. (eds) Handbook of Exoplanets . Springer, Cham. https://doi.org/10.1007/978-3-319-30648-3_10-1

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  • DOI: https://doi.org/10.1007/978-3-319-30648-3_10-1

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  • Publisher Name: Springer, Cham

  • Print ISBN: 978-3-319-30648-3

  • Online ISBN: 978-3-319-30648-3

  • eBook Packages: Springer Reference Physics & AstronomicsReference Module Physical and Materials Science