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ISOPHOT Surveys and the Extragalactic Background

Published online by Cambridge University Press:  13 May 2016

D. Lemke ,
P. Ábrahám ,
M. Haas ,
P. Héraudeau ,
S. Hotzel ,
C. Kiss ,
U. Klaas ,
O. Krause ,
C. Leinert  and
K. Meisenheimer
...Show all authors
D. Lemke
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
P. Ábrahám
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
M. Haas
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
P. Héraudeau
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
S. Hotzel
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
C. Kiss
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
U. Klaas
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
O. Krause
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
C. Leinert
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
K. Meisenheimer
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
M. Stickel
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
L. V. Tóth
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
M. Juvela
Affiliation:
University of Helsinki, Observatory, Helsinki, Finland
K. Mattila
Affiliation:
University of Helsinki, Observatory, Helsinki, Finland
R. Chini
Affiliation:
Ruhr-Universität Bochum, Astronomisches Institut, D-44780 Bochum, Germany
S. A. H. Müller
Affiliation:
Ruhr-Universität Bochum, Astronomisches Institut, D-44780 Bochum, Germany
M. J. D. Linden-Vørnle
Affiliation:
Niels Bohr Institute for Astronomy, Physics and Geophysics, Astronomical Observatory, Copenhagen, Denmark
H. U. Nørgaard-Nielsen
Affiliation:
Niels Bohr Institute for Astronomy, Physics and Geophysics, Astronomical Observatory, Copenhagen, Denmark

Abstract

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The higher spatial resolution and sensitivity of ISO allowed several extragalactic surveys to be extended to greater depth than obtained with IRAS. With the extended wavelength range deep surveys were performed for the first time at wavelengths up to ~ 200 μm. They favour galaxy models with strong evolution. With ISO's new capabilities the spectral energy distributions of larger samples of ULIRGs in the local universe and those of quasars and radio galaxies were determined. These data are applicable as templates to the more distant universe. Foreground components from zodiacal light and cirrus to the intracluster dust emission were studied in connection with their separation from the extragalactic background radiation.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 204: The Extragalactic Infrared Background and its Cosmological Implication , 2001 , pp. 247 - 259
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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