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I discuss the classical cosmological tests-- angular size-redshift, flux-redshift, and galaxy number counts-- in the light of the cosmology prescribed by the intepretation of CMB anisotropies. The discussion is somewhat of a primer for physicists, with emphasis upon the possible systematic uncertainties in the observations and their interpretation. Given the curious composition of the Universe inherent in the emerging cosmological model, I stress the value of searching for inconsistencies rather than concordance, and suggest that the prevailing mood of triumphalism in cosmology is premature.
35 pages, 13 figures, talk given at Second Aegean Summer School on the Early Universe
High Energy Physics - Theory, IA SUPERNOVAE, GRAVITATIONAL LENS B1608+656, SIZE REDSHIFT RELATION, Astrophysics (astro-ph), HUBBLE DEEP FIELD, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, General Relativity and Quantum Cosmology, MASS MODELS, PRIMORDIAL ABUNDANCE, CONSTANT, High Energy Physics - Theory (hep-th), LUMINOSITY FUNCTION, PROBE WMAP OBSERVATIONS, DARK ENERGY
High Energy Physics - Theory, IA SUPERNOVAE, GRAVITATIONAL LENS B1608+656, SIZE REDSHIFT RELATION, Astrophysics (astro-ph), HUBBLE DEEP FIELD, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics, General Relativity and Quantum Cosmology, MASS MODELS, PRIMORDIAL ABUNDANCE, CONSTANT, High Energy Physics - Theory (hep-th), LUMINOSITY FUNCTION, PROBE WMAP OBSERVATIONS, DARK ENERGY
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