RA/Dec (J2000) = 09h 50m 39.96s, +79° 01′ 49.7″ +/- 4.2 (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Source 1 has been manually confirmed as the GRB afterglow so these products are no longer updated.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 |
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We expect ~1.82×10-3 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 | 8.8 (±1.6) ×10-3 ct s-1 |
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Mean XRT count rate | 8.1 (±1.4) ×10-3 ct s-1 |
RASS upper limit | 0.03 ct s-1 |
Fading? | Yes |
Mean flux (Observed, 0.3—10 keV) | 2.6 (±0.5) ×10-13 erg cm-2s-1 |
Peak flux (Observed, 0.3—10 keV) | 2.9 (±0.5) ×10-13 erg cm-2s-1 |
Mean rate (PSPC equivalent) | 4.8 (±0.8) ×10-3 |
Peak rate (PSPC equivalent) | 5.2 (±0.9) ×10-3 |