RA/Dec (J2000) = 14h 19m 55.09s, -69° 21′ 13.1″ +/- 4.3 (radius, 90%) 
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Source 1 has been manually confirmed as the GRB afterglow so these products are no longer updated. The up-to-date data for the afterglow are now available through the main GRB results area for this GRB.
This is the probable afterglow because:
| Light curve | Spectrum |
|---|---|
We expect ~1.10×10-3 serendipitous objects at least as bright as this source in this tiled dataset, based on the logN-logS distribution of Mateos et al. (2008) [More details]
| Peak XRT count rate | 9.4 (±1.7) ×10-3 ct s-1 |
|---|---|
| Mean XRT count rate | 7.9 (±1.3) ×10-3 ct s-1 |
| RASS upper limit | 0.04 ct s-1 |
| Fading? | No |
| Mean flux (Observed, 0.3—10 keV) | 3.6 (±0.6) ×10-13 erg cm-2s-1 |
| Peak flux (Observed, 0.3—10 keV) | 4.3 (±0.8) ×10-13 erg cm-2s-1 |
| Mean rate (PSPC equivalent) | 5.9 (±1.0) ×10-3 |
| Peak rate (PSPC equivalent) | 7.0 (±1.3) ×10-3 |