User contributions
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- 12:57, 7 October 2012 (diff | hist) . . (+1) . . Light and distances (→Problem 17: the maximum in Friedman models) (current)
- 12:57, 7 October 2012 (diff | hist) . . (+154) . . Light and distances (→Problem 17: the maximum in Friedman models)
- 12:54, 7 October 2012 (diff | hist) . . (+740) . . Light and distances (→Problem 17: the maximum in Friedman models)
- 12:28, 7 October 2012 (diff | hist) . . (+49) . . Light and distances (→Problem 12: angular diameter distance in terms of redshift)
- 12:25, 7 October 2012 (diff | hist) . . (-7) . . Light and distances (→Problem 6: generalization to arbitrary curvature)
- 12:21, 7 October 2012 (diff | hist) . . (+180) . . Light and distances (→Problem 6: generalization to arbitrary curvature)
- 12:06, 7 October 2012 (diff | hist) . . (+74) . . Light and distances (→Problem 6: generalization to arbitrary curvature)
- 11:59, 7 October 2012 (diff | hist) . . (+1) . . Light and distances (→Problem 5: luminosity distance in a flat Universe)
- 11:57, 7 October 2012 (diff | hist) . . (+412) . . Light and distances
- 11:50, 7 October 2012 (diff | hist) . . (+383) . . Light and distances
- 10:27, 7 October 2012 (diff | hist) . . (+696) . . Light and distances
- 10:15, 7 October 2012 (diff | hist) . . (+684) . . Light and distances
- 14:59, 5 October 2012 (diff | hist) . . (+1) . . Light and distances (→Problem 17: the maximum in Friedman models)
- 14:58, 5 October 2012 (diff | hist) . . (+7) . . Light and distances (→Problem 11: the closed and open dusty Universes)
- 14:57, 5 October 2012 (diff | hist) . . (+558) . . Light and distances
- 14:51, 5 October 2012 (diff | hist) . . (+553) . . Light and distances
- 14:44, 5 October 2012 (diff | hist) . . (+130) . . Light and distances
- 14:42, 5 October 2012 (diff | hist) . . (+151) . . Light and distances
- 14:39, 5 October 2012 (diff | hist) . . (+31) . . Light and distances (→Problem 7: multi-component flat Universe)
- 14:39, 5 October 2012 (diff | hist) . . (+64) . . Light and distances (→Problem 7: multi-component flat Universe)
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