Background-source separation in astronomical images with bayesian probability 
theory - I. The method

Guglielmetti, F.; Fischer, R.; Dose, V.

doi:10.1111/j.1365-2966.2009.14739.x

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Background-source separation in astronomical images with bayesian probability theory - I. The method

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Guglielmetti, F.
Material Research (MF), Max Planck Institute for Plasma Physics, Max Planck Society;

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Fischer, R.
Tokamak Edge and Divertor Physics (E2), Max Planck Institute for Plasma Physics, Max Planck Society;

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Guglielmetti, F., Fischer, R., & Dose, V. (2009). Background-source separation in astronomical images with bayesian probability theory - I. The method. Monthly Notices of the Royal Astronomical Society, 396(1), 165-190. doi:10.1111/j.1365-2966.2009.14739.x.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0026-F532-D

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