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VIRUS-W A fiber based integral field unit spectrograph for the study of galaxy bulges

Published online by Cambridge University Press:  01 July 2007

Maximilian H. Fabricius ,
Ralf Bender ,
Niv Drory ,
Frank Grupp ,
Gary J. Hill  and
Ulrich Hopp
Maximilian H. Fabricius
Affiliation:
University Observatory of the Ludwig-Maximilians University (LMU), Munich, Germany Max-Planck Institute for Extraterrestrial Physics (MPE), Munich, Germany
Ralf Bender
Affiliation:
University Observatory of the Ludwig-Maximilians University (LMU), Munich, Germany Max-Planck Institute for Extraterrestrial Physics (MPE), Munich, Germany
Niv Drory
Affiliation:
University Observatory of the Ludwig-Maximilians University (LMU), Munich, Germany Max-Planck Institute for Extraterrestrial Physics (MPE), Munich, Germany
Frank Grupp
Affiliation:
University Observatory of the Ludwig-Maximilians University (LMU), Munich, Germany
Gary J. Hill
Affiliation:
McDonald Observatory and Department of Astronomy, University of Texas at Austin, Austin, Texas, USA
Ulrich Hopp
Affiliation:
University Observatory of the Ludwig-Maximilians University (LMU), Munich, Germany Max-Planck Institute for Extraterrestrial Physics (MPE), Munich, Germany
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Abstract

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We presented the design for a fiber based integral field unit spectrograph for the new two meter class Wendelstein telescope in Bavaria, Germany. The proposed spectrograph will feature a fiberhead consisting of 246 individual optical fibers and a field of view of approximately 1′ × 2′ and two different spectral resolution modes optimized for the study of bulges of local late-type galaxies.

Keywords

galaxies: bulgesgalaxies: kinematics and dynamicsinstrumentation: spectrographs
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S245: Formation and Evolution of Galaxy Bulges , July 2007 , pp. 417 - 418
Copyright
Copyright © International Astronomical Union 2008

References

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