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Galaxy
structure – how is the mass in the
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universe
distributed (and recall gas can be
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important,
too!)? Homogeneous? On what
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scale?
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Text
is a bit old (fine for history), but the best
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newest
information will come from SDSS and
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2dF. CHECK IT OUT!
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Background
radiation also of interest (discrete
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sources
vs. true diffuse background).
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