MUSE (Multi Unit Spectroscopic Explorer) is a powerful integral-field spectrograph installed on the Very Large Telescope (VLT) at the Paranal Observatory in Chile. It allows astronomers to obtain spectra of an entire field of view at once, rather than just a single point. This creates a 3D data cube where two dimensions are spatial (image) and the third is spectral (wavelength). MUSE is used for a wide range of astronomical research, including studying the formation and evolution of galaxies, probing the structure of distant quasars, and mapping the dynamics of star clusters.
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