RA/Dec (J2000) = 21h 29m 38.59s, +37° 07′ 56.6″ +/- 3.8 (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Source 1 has been manually confirmed as the GRB afterglow so these products are no longer updated.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 ~2.00×10-3 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 | 0.109 (±0.025) ct s-1 | 
|---|---|
| Mean XRT count rate | 7.7 (±0.8) ×10-2 ct s-1 | 
| RASS upper limit | 0.03 ct s-1 | 
| Fading? | No | 
| Mean flux (Observed, 0.3—10 keV) | 3.5 (±0.4) ×10-12 erg cm-2s-1 | 
| Peak flux (Observed, 0.3—10 keV) | 4.9 (±1.1) ×10-12 erg cm-2s-1 | 
| Mean rate (PSPC equivalent) | 7.5 (±0.8) ×10-2 | 
| Peak rate (PSPC equivalent) | 0.105 (±0.024) |