TPF interferometer performance requirements

Details TPF interferometer performance requirements TPF interferometer performance requirements

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spie.5170...79n&link_type=abstract

Techniques and Instrumentation for Detection of Exoplanets. Edited by Coulter, Daniel R. Proceedings of the SPIE, Volume 5170,

Physics

1

Scientific paper

The TPF interferometer family suppresses the stellar glare using a deep interferometric null, which for the planet can become constructive interference because of its angular offset. The null depth need not be as great as the star-planet contrast, but its systematic fluctuations must be perhaps 5 times better than the variations which constitute the planet's signature. We present an allocation of errors which meet these needs, and identify areas which need better definition.

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