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Explore the cutting-edge technology behind MUSE, an integral field spectrograph built by a consortium of European institutes. Learn about the compact CCD head, low frequency pulse tube cooler, new general detector controller, and detector requirements.
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Slicing the UniverseCCDs for MUSE Roland Reissa, Sebastian Deiriesa, Jean Louis Lizona, Manfred Meyera, Javier Reyesa, Roland Baconb, François Hénaultb, Magali Loupiasb(a) European Southern Observatory (http://www.eso.org)Karl-Schwarzschild-Str. 2 D-85748 Garching by Munich, Germany(b) CRAL - Observatoire de Lyon, 9 avenue Charles André, 69230 Saint-Genis-Laval, France
Slicing the UniverseCCDs for MUSE • MUSE (Multi Unit Spectral Explorer) is built by a consortium of European institutes(ESO, Göttingen, Leiden, Lyon, Toulouse, Zürich). • 2nd generation instrument for the VLT. • Integral field spectrometer for the Nasmyth focus. • 24 Integral Field Units (IFU). • 24 cryostats with one 4k x 4k CCD attached to IFUs. Reiss et al., Slicing the Universe
Compact CCD Head • Low Frequency Pulse Tube Cooler. • Standard head for future ESO instruments. Reiss et al., Slicing the Universe
New General detector Controler (NGC) Reiss et al., Slicing the Universe
Detector Requirements Reiss et al., Slicing the Universe