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Thesis

Observing bright stars and their planets from the Earth and from space

Abstract:

The discovery and characterization of extrasolar planets is a leading frontier of science, which is limited by our ability to extract real astrophysical signals masked by systematic noise. In this Thesis I develop techniques for self-calibration in optical astronomy, in both imaging and photometry, applicable both to observations from the ground and for space telescopes, and apply these to searching for exoplanets.

Kernel phase interferometry is a method for improving high angular ...

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Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author

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Role:
Supervisor
Clarendon Fund More from this funder
Type of award:
DPhil
Level of award:
Doctoral
Awarding institution:
University of Oxford
Subjects:
UUID:
uuid:d692bf96-ccf8-47bf-b246-1bbedcce60e5
Deposit date:
2018-05-03

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