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Modelling high-z galaxies from the far-UV to the far-IR

Abstract:

In this paper, we report on a first estimate of the contribution of galaxies to the diffuse extragalactic background from the far-UV to the submm, based on semi--analytic models of galaxy formation and evolution. We conclude that the global multi--wavelength picture seems to be consistent provided a quite important fraction of star--formation be hidden in dust--enshrouded systems at intermediate and high--redshift. We show that, according to such models, galaxies cannot stand as important co...

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Publication status:
Published
Peer review status:
Peer reviewed

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Astrophysics
Guiderdoni, B More by this author
Publisher:
Editions Frontières
Journal:
Dwarf Galaxies And Cosmology Journal website
Publication date:
1998
URN:
uuid:1f188212-095b-42e2-8393-ccf88ec369f9
Source identifiers:
205772
Local pid:
pubs:205772
ISBN:
2863322389
Keywords:

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