RA/Dec (J2000) = 17h 21m 48.83s, +38° 19′ 04.6″ +/- 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Source 1 has been manually confirmed as the GRB afterglow so these products are no longer updated.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 |
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We expect ~4.50×10-5 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 | 1.1 (±0.3) ×10-2 ct s-1 |
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Mean XRT count rate | 1.03 (±0.17) ×10-2 ct s-1 |
RASS upper limit | 0.03 ct s-1 |
Fading? | Yes |
Mean flux (Observed, 0.3—10 keV) | 4.6 (±0.8) ×10-13 erg cm-2s-1 |
Peak flux (Observed, 0.3—10 keV) | 5.1 (±1.4) ×10-13 erg cm-2s-1 |
Mean rate (PSPC equivalent) | 1.07 (±0.18) ×10-2 |
Peak rate (PSPC equivalent) | 1.2 (±0.3) ×10-2 |