Journal
ASTROPHYSICAL JOURNAL
Volume 549, Issue 2, Pages 716-720Publisher
UNIV CHICAGO PRESS
DOI: 10.1086/319431
Keywords
cosmology : theory; relativity
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In this paper we use the integration scheme for the exact spherically symmetric Einstein field equations in observational coordinates recently developed by Araujo and Stoeger, and input data functions for area distance and galaxy number counts that would be obtained if the universe were exactly represented by nonflat Friedmann-Lemaitre-Robertson-Walker models.
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