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• |
Observed
Properties of Standard Objects in the Friedman
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World
Models with zero cosmological constant (cf. Hogg
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2000,
chapter 5, Ned Wright’s calculator).
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Angular
Diameters (need Angular Distance f(z))
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Flux
Densities (need luminosity distance f(z))
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Comoving
volume within redshift z
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In
particular covered in more detail in section 7.2.8
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