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(newest | oldest) View (newer 20 | older 20) (20 | 50 | 100 | 250 | 500)- 18:08, 25 November 2011 Gsawgwikiadmin talk contribs uploaded File:AroundGaiaPoster2011.pdf
- 15:42, 22 November 2011 Lukasz talk contribs uploaded a new version of File:GSAFSManual2011.pdf
- 13:18, 22 November 2011 User account Giuseppe.Altavilla talk contribs was created by Gsawgwikiadmin talk contribs
- 14:38, 20 November 2011 Lukasz talk contribs uploaded File:GSAFSManual2011.pdf
- 13:37, 3 November 2011 Lukasz talk contribs uploaded File:Example.png
- 13:36, 3 November 2011 Lukasz talk contribs uploaded File:GaiaAlertsVerificationTimeline.png
- 13:08, 3 November 2011 Lukasz talk contribs uploaded File:GaiaAlertsVerificationTimeline.pdf
- 21:10, 19 September 2011 Lukasz talk contribs uploaded a new version of File:Whitebook2011.pdf
- 15:51, 18 September 2011 Lukasz talk contribs uploaded File:Whitebook2011.pdf (The Whitebook 2011.)
- 14:27, 13 September 2011 Sth talk contribs uploaded File:Gaia sne.png
- 14:24, 13 September 2011 Sth talk contribs uploaded File:Gaia sne.pdf (predictions for SNe detections as a function of magnitude)
- 14:17, 13 September 2011 Sth talk contribs uploaded File:Supernovae alerts.pdf (predictions for SNe alerts with the new scanning law - from Hodgkin & Belokurov.)
- 14:59, 11 September 2011 Jure.Japelj talk contribs uploaded File:M star spectrum.png
- 10:58, 8 September 2011 Jure.Japelj talk contribs uploaded File:Yzcmi spec.png
- 10:54, 8 September 2011 Jure.Japelj talk contribs uploaded File:Yzcmi.png
- 10:41, 8 September 2011 Jure.Japelj talk contribs uploaded File:Cn leo.png
- 10:36, 8 September 2011 Jure.Japelj talk contribs uploaded File:Uv ceti.png
- 10:35, 8 September 2011 Jure.Japelj talk contribs uploaded File:Gj3332.png
- 11:02, 15 July 2011 Jure.Japelj talk contribs uploaded File:F10.png (Left: Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change of magnitude in the time in which an afterglow is in the entire field of view (red) for the on-axis case. Right: Distrib)
- 11:01, 15 July 2011 Jure.Japelj talk contribs uploaded 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)