MUSE Dream Conclusion: The Sky Verdict

被引：4

作者：

Caillier, P. ^{[1
]}

Accardo, M. ^{[4
]}

Adjali, L. ^{[1
]}

Anwand, H. ^{[5
]}

Bacon, R. ^{[1
]}

Boudon, D. ^{[1
]}

Capoani, L. ^{[1
]}

Daguise, E. ^{[1
]}

Dupieux, M. ^{[6
]}

Dupuy, C. ^{[4
]}

Francois, M. ^{[1
]}

Glindemann, A. ^{[4
]}

Gojak, D. ^{[4
]}

Gonte, F. ^{[9
,10
]}

Haddad, N. ^{[9
,10
]}

Hansali, G. ^{[1
]}

Hahn, T. ^{[2
]}

Jarno, A. ^{[1
]}

Kelz, A. ^{[2
]}

Koehler, C. ^{[5
]}

Kosmalski, J. ^{[1
]}

Laurent, F.

Larrieu, M. ^{[6
]}

Lizon, J. -L. ^{[4
]}

Loupias, M. ^{[1
]}

Manescau, A. ^{[4
]}

Migniau, J. E. ^{[1
]}

Monstein, C. ^{[3
]}

Nicklas, H. ^{[5
]}

Pares, L. ^{[6
]}

Pecontal-Rousset, A. ^{[1
]}

Piqueras, L. ^{[1
]}

Reiss, R. ^{[4
]}

Remillieux, A. ^{[1
]}

Renault, E. ^{[1
]}

Rupprecht, G. ^{[4
]}

Streicher, O. ^{[2
]}

Stuik, R. ^{[7
]}

Valentin, H. ^{[6
]}

Vernet, J. ^{[4
]}

Weilbacher, P. ^{[2
]}

Zins, G. ^{[8
]}

机构：

[1] Univ Claude Bernard Lyon I, CNRS, Ctr Rech Astrophys Lyon, 9 Ave Charles Andre, F-69230 St Genis Laval, France

[2] Leibniz Inst AIP, D-14482 Potsdam, Germany

[3] Swiss Fed Inst Technol, Inst Astron, Dept Phys, CH-8093 Zurich, Switzerland

[4] European Southern Observat, D-85748 Garching, Germany

[5] Univ Gottingen, Inst Astrophys, D-37077 Gottingen, Germany

[6] Univ Grenoble 1, CNRS, Inst Res Astrophys Planetol, Observ Midi Pyrenees, F-31400 Toulouse, France

[7] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[8] Univ Grenoble 1, CNRS, Inst Planetol Astrophys, Grenoble, France

[9] Paranal Observ, European Southern Observ, Munich, Germany

[10] European So Observ, Munich, Germany

来源：

MODELING, SYSTEMS ENGINEERING, AND PROJECT MANAGEMENT FOR ASTRONOMY VI | 2014年 / 9150卷

关键词：

MUSE instrument; project management; development; PBS; WBS; IFU; Integral Field; 3D spectroscopy;

D O I：

10.1117/12.2056845

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

MUSE (Multi Unit Spectroscopic Explorer) is a second generation instrument built for ESO (European Southern Observatory). The MUSE project is supported by a European consortium of 7 institutes. After the finalisation of its integration in Europe, the MUSE instrument has been partially dismounted and shipped to the VLT (Very Large Telescope) in Chile. From October 2013 till February 2014, it has then been reassembled, tested and finally installed on the telescope its final home. From there it collects its first photons coming from the outer limit of the visible universe. This critical moment when the instrument finally meets its destiny is the opportunity to look at the overall outcome of the project and the final performance of the instrument on the sky. The instrument which we dreamt of has become reality. Are the dreamt performances there as well? These final instrumental performances are the result of a step by step process of design, manufacturing, assembly, test and integration. Now is also time to review the path opened by the MUSE project. What challenges were faced during those last steps, what strategy, what choices did pay off? What did not?

引用

页数：16

共 8 条

[1]

BACON R, 2006, P SPIE, V6269

[2]

Caillier P., 2012, P SPIE, P8449

[3]

Caillier P., 2014, P SPIE, P9147

[4]

Caillier P., 2010, P SPIE, P7738

[5]

Laurent F., 2012, P SPIE, V8446-226

[6]

Laurent F., 2014, P SPIE, V9151-64

[7]

Loupias M., 2012, P SPIE, P8446

[8]

Remillieux A., 2012, P SPIE, V8450-137

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