Abstract: Duchamp is 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.
Credit: Whiting, Matthew
Site: https://www.atnf.csiro.au/people/Matthe ... g/Duchamp/
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2012MNRAS.421.3242W