1201.2710 (Matthew T. Whiting)
Matthew T. Whiting
This paper describes the Duchamp source finder, a piece of software designed
to find and describe sources in 3-dimensional, spectral-line data cubes.
Duchamp has been developed with HI (neutral hydrogen) observations in mind, but
is widely applicable to many types of astronomical images. It features
efficient source detection and handling methods, noise suppression via
smoothing or multi-resolution wavelet reconstruction, and a range of graphical
and text-based outputs to allow the user to understand the detections. This
paper details some of the key algorithms used, and illustrates the
effectiveness of the finder on different data sets.
View original:
http://arxiv.org/abs/1201.2710
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