1. The MUSE second-generation VLT instrument
- Author
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Christophe Dupuy, E. Popow, T. Contini, Stefan Dreizler, Roland Reiss, Marc François, Jean-Pierre Dubois, G. Gallou, L. Adjali, T. Hahn, L. Capoani, Christian Monstein, Lutz Wisotzki, Andreas Kelz, A. Remillieux, E. Renault, C. Koehler, C. Petit, S. Brau-Nogué, G. Hansali, M. Dupieux, Johan Kosmalski, Andreas Glindemann, T. Fechner, Ole Streicher, P. Caillier, T. Gharsa, Jarle Brinchmann, Joel Vernet, M. Le Floc'h, G. Soucail, Matteo Accardo, J.-L. Lizon, Remko Stuik, I. Biswas, B. Guiderdoni, Simon J. Lilly, S. Deiries, H. Anwand, Svend-Marian Bauer, Harald Nicklas, Joop Schaye, Antonio Manescau, F. Laurent, C. M. Carollo, Roland Bacon, Eric Emsellem, E. Daguisé, D. Boudon, Denis Serre, Aurélien Jarno, P. Couderc, Jeremy Blaizot, A. Fleischmann, Martin Roth, Roser Pello, N. Yerle, D. Gojak, J.-C. Olaya, Valentin H, M. Loupias, Gero Rupprecht, B. Delabre, Luca Pasquini, Matthias Steinmetz, L. Parès, Arlette Pécontal-Rousset, and Peter M. Weilbacher
- Subjects
Computer science ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,01 natural sciences ,law.invention ,Optics ,Integral field spectrograph ,law ,0103 physical sciences ,Astrophysics::Solar and Stellar Astrophysics ,Adaptive optics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,010303 astronomy & astrophysics ,Spectrograph ,Astrophysics::Galaxy Astrophysics ,010308 nuclear & particles physics ,business.industry ,System of measurement ,Detector ,Astrophysics::Instrumentation and Methods for Astrophysics ,Laser ,Multi Unit Spectroscopic Explorer ,Stars ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics ,business - Abstract
The Multi Unit Spectroscopic Explorer (MUSE) is a second-generation VLT panoramic integral-field spectrograph currently in manufacturing, assembly and integration phase. MUSE has a field of 1x1 arcmin2 sampled at 0.2x0.2 arcsec2 and is assisted by the VLT ground layer adaptive optics ESO facility using four laser guide stars. The instrument is a large assembly of 24 identical high performance integral field units, each one composed of an advanced image slicer, a spectrograph and a 4kx4k detector. In this paper we review the progress of the manufacturing and report the performance achieved with the first integral field unit., Comment: 10 pages, 5 figures
- Published
- 2010
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