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2D–1D Wavelet Reconstruction as a Tool for Source Finding in Spectroscopic Imaging Surveys

Published online by Cambridge University Press:  02 January 2013

L. Flöer  and
B. Winkel
L. Flöer*
Affiliation:
Argelander-Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany
B. Winkel
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
*
CCorresponding author. Email: lfloeer@astro.uni-bonn.de
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Abstract

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Today, image denoising by thresholding of wavelet coefficients is a commonly used tool for 2D image enhancement. Since the data product of spectroscopic imaging surveys has two spatial dimensions and one spectral dimension, the techniques for denoising have to be adapted to this change in dimensionality. In this paper we will review the basic method of denoising data by thresholding wavelet coefficients and implement a 2D–1D wavelet decomposition to obtain an efficient way of denoising spectroscopic data cubes. We conduct different simulations to evaluate the usefulness of the algorithm as part of a source finding pipeline.

Keywords

methods: data analysistechniques: image processingtechniques: spectroscopic
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 29 , Special Issue 3: Source Finding and Visualisation , 2012 , pp. 244 - 250
Copyright
Copyright © Astronomical Society of Australia 2012

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