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Latest revision as of 11:01, 15 July 2011
Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results are given for a time of five years.
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| current | 11:01, 15 July 2011 |  | 800 × 568 (53 KB) | Jure.Japelj (talk | contribs) | Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results |
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