File list
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Date | Name | Thumbnail | Size | User | Description | Versions |
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13:36, 3 November 2011 | GaiaAlertsVerificationTimeline.png (file) | 45 KB | Lukasz | 1 | ||
13:08, 3 November 2011 | GaiaAlertsVerificationTimeline.pdf (file) | 42 KB | Lukasz | 1 | ||
21:10, 19 September 2011 | Whitebook2011.pdf (file) | 121 KB | Lukasz | 2 | ||
14:27, 13 September 2011 | Gaia sne.png (file) | 53 KB | Sth | 1 | ||
14:24, 13 September 2011 | Gaia sne.pdf (file) | 64 KB | Sth | predictions for SNe detections as a function of magnitude | 1 | |
14:17, 13 September 2011 | Supernovae alerts.pdf (file) | 108 KB | Sth | predictions for SNe alerts with the new scanning law - from Hodgkin & Belokurov. | 1 | |
14:59, 11 September 2011 | M star spectrum.png (file) | 34 KB | Jure.Japelj | 1 | ||
10:58, 8 September 2011 | Yzcmi spec.png (file) | 19 KB | Jure.Japelj | 1 | ||
10:54, 8 September 2011 | Yzcmi.png (file) | 27 KB | Jure.Japelj | 1 | ||
10:41, 8 September 2011 | Cn leo.png (file) | 24 KB | Jure.Japelj | 1 | ||
10:36, 8 September 2011 | Uv ceti.png (file) | 48 KB | Jure.Japelj | 1 | ||
10:35, 8 September 2011 | Gj3332.png (file) | 12 KB | Jure.Japelj | 1 | ||
11:02, 15 July 2011 | F10.png (file) | 49 KB | Jure.Japelj | 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 | 1 | |
11:01, 15 July 2011 | F6.png (file) | 53 KB | Jure.Japelj | 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 | 1 | |
11:00, 15 July 2011 | F5.png (file) | 63 KB | Jure.Japelj | 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. | 1 | |
09:24, 1 July 2011 | GaiaAlertsWorkshop-June2011.jpg (file) | 3.68 MB | Lukasz | 1 | ||
09:12, 1 July 2011 | Galaxies.jpg (file) | 12 KB | Gaia | 1 | ||
20:06, 31 March 2011 | Theta2.png (file) | 1 KB | Jure.Japelj | 1 | ||
20:06, 31 March 2011 | Theta1.png (file) | 1 KB | Jure.Japelj | 1 | ||
20:05, 31 March 2011 | Thetaobs.png (file) | 808 bytes | Jure.Japelj | 1 | ||
20:02, 31 March 2011 | Theta.png (file) | 510 bytes | Jure.Japelj | 1 | ||
16:38, 31 March 2011 | Report.pdf (file) | 324 KB | Jure.Japelj | Report on the simulation of the detectability of regular 'on-axis' GRB optical afterglows with the Gaia satellite. | 1 | |
14:49, 31 March 2011 | F4.jpg (file) | 29 KB | Jure.Japelj | 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). | 1 | |
14:48, 31 March 2011 | F3.jpg (file) | 35 KB | Jure.Japelj | 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). | 1 | |
14:47, 31 March 2011 | F2.jpg (file) | 32 KB | Jure.Japelj | The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments. | 1 | |
14:46, 31 March 2011 | F1.jpg (file) | 23 KB | Jure.Japelj | The average GRB on-axis afterglow detection rate in five years. | 1 | |
14:45, 31 March 2011 | Kann.png (file) | 362 KB | Jure.Japelj | A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. | 1 | |
10:20, 31 March 2011 | F1.pdf (file) | 8 KB | Jure.Japelj | 2 | ||
18:52, 30 March 2011 | Kann afterglow1.pdf (file) | 232 KB | Jure.Japelj | A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. | 1 | |
18:50, 30 March 2011 | Kann afterglow.pdf (file) | 232 KB | Jure.Japelj | A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. | 3 | |
16:54, 28 March 2011 | GaiaWorkshop2011poster.pdf (file) | 1.7 MB | Gsawgwikiadmin | 1 | ||
16:53, 28 March 2011 | Nature09724-s1.pdf (file) | 238 KB | Gaia | 1 | ||
16:53, 28 March 2011 | Poster.jpg (file) | 644 KB | Gsawgwikiadmin | 1 | ||
16:37, 28 March 2011 | Nophoto.jpg (file) | 2 KB | Gaia | 1 | ||
15:56, 2 February 2011 | Gilmore09 GBOG M05 CU5 GG.pdf (file) | 1.45 MB | Lukasz | Gilmore's presentation on GBOG and Alerts Verification | 1 | |
11:46, 28 October 2010 | XrayBin-Sturm2010.png (file) | 115 KB | Lukasz | 1 | ||
15:53, 22 October 2010 | Postgsaw wb.pdf (file) | 1.96 MB | Lukasz | 1 | ||
10:14, 9 September 2010 | Uaf.pdf (file) | 49 KB | Gaia | For testing upload | 1 | |
11:11, 12 July 2010 | Popowski2005-Gaia Science Alerts.pdf (file) | 639 KB | Lukasz | 1 | ||
15:23, 6 July 2010 | Gsaw-abstract book.pdf (file) | 58 KB | Lukasz | 5 | ||
09:03, 2 July 2010 | GaiaScienceAlertsWorkshop2010photo small.jpg (file) | 93 KB | Lukasz | 1 | ||
15:30, 24 June 2010 | GaiaScienceAlertsWorkshop2010photo.jpg (file) | 420 KB | Lukasz | 3 | ||
14:33, 15 June 2010 | Screen shot 2010-06-15 at 14.32.12.png (file) | 129 KB | Sth | 1 | ||
14:25, 15 June 2010 | GAIA-info-reverse.jpg (file) | 359 KB | Sth | Map of the Ioa and Churchill | 1 | |
10:48, 15 June 2010 | 130410InfoforGuests.pdf (file) | 58 KB | Sth | Information for guests of Churchill College (2 pages) | 1 | |
11:41, 4 June 2010 | Gog sampling.png (file) | 37 KB | Lukasz | 1 | ||
15:58, 30 March 2010 | GAIA-2010web-poster.jpg (file) | 422 KB | Lukasz | 2 | ||
10:59, 22 March 2010 | GAIA-2010web.jpg (file) | 175 KB | Lukasz | 1 | ||
20:53, 4 March 2010 | Churchill2.jpg (file) | 2.53 MB | Lukasz | 1 | ||
20:48, 4 March 2010 | Churchill1.jpg (file) | Error creating thumbnail: File with dimensions greater than 12.5 MP |
1.29 MB | Lukasz | 1 |