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From Gaia Science Alerts Working Group
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- 15:12, 31 March 2011 diff hist +2 Triggers:GRBs
- 15:11, 31 March 2011 diff hist -11 Triggers:GRBs
- 15:10, 31 March 2011 diff hist +9 Triggers:GRBs
- 15:09, 31 March 2011 diff hist -5 Triggers:GRBs
- 15:05, 31 March 2011 diff hist +4 Triggers:GRBs
- 15:05, 31 March 2011 diff hist -12 Triggers:GRBs
- 15:04, 31 March 2011 diff hist +25 Triggers:GRBs
- 15:03, 31 March 2011 diff hist -14 Triggers:GRBs
- 15:03, 31 March 2011 diff hist +4 Triggers:GRBs
- 15:02, 31 March 2011 diff hist -9 Triggers:GRBs
- 15:02, 31 March 2011 diff hist +4 Triggers:GRBs
- 14:59, 31 March 2011 diff hist -2 Triggers:GRBs
- 14:58, 31 March 2011 diff hist +13 Triggers:GRBs
- 14:56, 31 March 2011 diff hist -2 Triggers:GRBs
- 14:56, 31 March 2011 diff hist +1,299 Triggers:GRBs
- 14:49, 31 March 2011 diff hist +187 N File:F4.jpg Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray). current
- 14:48, 31 March 2011 diff hist +222 N File:F3.jpg Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red). current
- 14:47, 31 March 2011 diff hist +116 N File:F2.jpg The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments. current
- 14:46, 31 March 2011 diff hist +63 N File:F1.jpg The average GRB on-axis afterglow detection rate in five years. current