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From Gaia Science Alerts Working Group
Jump to navigationJump to search- 11:01, 15 July 2011 diff hist +291 N File:F6.png 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 current
- 11:00, 15 July 2011 diff hist +191 N File:F5.png GRB on-axis and OAs detection rate in five years of Gaia's operation as a function of limiting magnitude. In the case of OAs, the results are given for two different circumburst environments. current
- 14:14, 5 April 2011 diff hist +47 Triggers:GRBs →Simulation references
- 14:13, 5 April 2011 diff hist -9 Triggers:GRBs →Simulation references
- 14:10, 5 April 2011 diff hist -1 Triggers:GRBs →Simulation references
- 14:10, 5 April 2011 diff hist +56 Triggers:GRBs →Simulation references
- 13:07, 5 April 2011 diff hist -127 Triggers:GRBs
- 13:06, 5 April 2011 diff hist +14 Triggers:GRBs
- 13:05, 5 April 2011 diff hist -4 Triggers:GRBs
- 13:04, 5 April 2011 diff hist +118 Triggers:GRBs
- 20:08, 31 March 2011 diff hist +2 Triggers:GRBs
- 20:07, 31 March 2011 diff hist -29 Triggers:GRBs
- 20:06, 31 March 2011 diff hist 0 N File:Theta2.png current
- 20:06, 31 March 2011 diff hist 0 N File:Theta1.png current
- 20:05, 31 March 2011 diff hist 0 N File:Thetaobs.png current
- 20:02, 31 March 2011 diff hist +8 Triggers:GRBs
- 20:02, 31 March 2011 diff hist 0 N File:Theta.png current
- 20:01, 31 March 2011 diff hist -32 Triggers:GRBs
- 19:58, 31 March 2011 diff hist 0 Triggers:GRBs
- 19:58, 31 March 2011 diff hist +31 Triggers:GRBs