Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-06-13
Astronomy and Astrophysics
Astrophysics
6 pages, 4 figures. This paper will be published in the proceedings of the conference Space Telescopes and Instrumentation I:
Scientific paper
10.1117/12.670553
To detect Earth-like planets in the visible with a coronagraphic telescope, two major noise sources have to be overcome: the photon noise of the diffracted star light, and the speckle noise due to the star light scattered by instrumental defects. Coronagraphs tackle only the photon noise contribution. In order to decrease the speckle noise below the planet level, an active control of the wave front is required. We have developed analytical methods to measure and correct the speckle noise behind a coronagraph with a deformable mirror. In this paper, we summarize these methods, present numerical simulations, and discuss preliminary experimental results obtained with the High-Contrast Imaging Testbed at NASA's Jet Propulsion Laboratory.
Borde Pascal J.
Kern Brian D.
Kuhnert Andreas C.
Traub Wesley A.
Trauger John T.
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