Constraining the Dark Matter Distribution With Large-Scale Structure Observations

Details Constraining the Dark Matter Distribution With Large-Scale Structure Observations Constraining the Dark Matter Distribution With Large-Scale Structure Observations

1998-09-02

arxiv.org/abs/astro-ph/9809023v1

Astronomy and Astrophysics

Astrophysics

To appear in "Astrophysics with Infrared Surveys: A Prelude to SIRTF," PASP Conference Proceedings, 10 pages, 2 figures

Scientific paper

We discuss the use of galaxies to trace the large-scale structure of the
universe and thereby to make cosmological inferences. We put special emphasis
on our lack of knowledge about the relative distribution of galaxies and the
dynamically important dark matter. We end with a discussion of the increasing
importance of infrared astronomy to large-scale structure studies.

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