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Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S299(8), p. 350-351

DOI: 10.1017/s1743921313008909

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First High-Angular Resolution L' Images of the β Pictoris Debris Disc with the VLT / NaCo

This paper is available in a repository.
This paper is available in a repository.

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Data provided by SHERPA/RoMEO

Abstract

AbstractImaging debris discs in the L′-band (3.8 μm) is a difficult task. Quasi-static speckles from imperfect optics prevail below 1″ whereas background emission is the dominant noise source beyond that separation and is much larger than at shorter wavelengths. We demonstrate here the potential of the newly commissioned AGPM coronograph on VLT/NaCo combined with advanced star and sky subtraction technique based on Principal Component Analysis, and we analyze the morphology of the β Pictoris disc.