The second generation VLT instrument MUSE: Science drivers and instrument design

Conference item

The Multi Unit Spectroscopic Explorer (MUSE) is a second generation VLT panoramic integral-field spectrograph operating in the visible wavelength range. MUSE has a field of 1x1 arcmin(2) sampled at 0.20.2 arcsec(2) and is assisted by a ground layer adaptive optics system using four laser guide stars. The simultaneous spectral range is 0.465-0.93 mum, at a resolution of Rsimilar to3000. MUSE couples the discovery potential of a large imaging device to the measuring capabilities of a high-quality spectrograph, while taking advantage of the increased spatial resolution provided by adaptive optics. This makes MUSE a unique and tremendously powerful instrument for discovering and characterizing objects that lie beyond the reach of even the deepest imaging surveys. MUSE has also a high spatial resolution mode with 7.5x7.5 arcsec(2) field of view sampled at 25 milli-arcsec. In this mode MUSE should be able to get diffraction limited data-cube in the 0.6-1 mum wavelength range. Although MUSE design has been optimized for the study of galaxy formation and evolution, it has a wide range of possible applications; e.g. monitoring of outer planets atmosphere, young stellar objects environment, supermassive black holes and active nuclei in nearby galaxies or massive spectroscopic survey of stellar fields.

Authors: Bacon, R; Bauer, S; Bower, R; Cabrit, S; Cappellari, M

• Publication status: Published
• Journal: GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3
• Volume: 5492
• Issue: PART 2
• Pages: 1145-1149
• Publication date: 2004-01-01
• Event title: Conference on Ground-based Instrumentation for Astronomy
• DOI: 10.1117/12.549009
• ISSN: 0277-786X
• ISBN: 0819454249