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Loading contentA spectrograph that records a full spectrum at every point in a two-dimensional field of view at once, producing a 'data cube' of the sky — an image where every pixel is a spectrum. It maps how motion and composition vary across a galaxy or nebula in a single exposure; MUSE on the VLT is a leading example.
Facts on this topic will be cited from these primary and reference sources.
Southern-hemisphere observatory data and imagery (VLT, ALMA partner).