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Galaxy
distributions seen in images are 2-d
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projections
on the sky.
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Need
distances…easiest way is to use the
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Hubble
flow and redshifts, either
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photometric
or spectra (best).
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Reminder
– SDSS and 2dF rule here now.
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Huchra
and Gellar’s “Z-machine” for the
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CfA
survey as recounted in “Lonely Hearts
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of
the Cosmos” by Dennis Overbye – Great!
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