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The Promise of Multiwavelength and IFU Observations

Published online by Cambridge University Press:  13 April 2010

Robert C. Kennicutt Jr. ,
Cai-Na Hao ,
Benjamin D. Johnson ,
Fabian Rosales-Ortega ,
Angeles Díaz ,
Anna Pasquale  and
Sebastian F. Sánchez
Robert C. Kennicutt Jr.
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
Cai-Na Hao
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
Benjamin D. Johnson
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
Fabian Rosales-Ortega
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK
Angeles Díaz
Affiliation:
Departamento de Física Teórica, C-XI, Universidad Autónoma de Madrid, 28049 Madrid, Spain
Anna Pasquale
Affiliation:
Max-Planck Institute für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
Sebastian F. Sánchez
Affiliation:
Centro Astronómico Hispano Alemám, Calar Alto, CSIC-MPG, Jesús Durbán Remón 2, E-04004, Almeria, Spain
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Abstract

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Many of the advances of the last decade in this subject have been the result of large spectroscopic surveys of galaxies on the one hand, and multi-wavelength surveys of galaxies on the other. This talk highlights applications that exploit a combination of spectroscopic and multi-wavelength diagnostics. Most applications to date have been based on spatially integrated measurements of galaxies, but the introduction of wide-field integral field spectrometers promises to extend ths approach to spatially-resolved analyses of galaxies.

Keywords

dustextinctiongalaxies: ISMgalaxies: stellar contentinfrared: galaxiesultraviolet: galaxiestechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 217 - 224
Copyright
Copyright © International Astronomical Union 2010

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