RA/Dec (J2000) = 19h 09m 40.04s, +36° 55′ 03.0″ +/- 3.9 (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Source 1 has been manually confirmed as the GRB afterglow so these products are no longer updated.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 ~3.97×10-5 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 | 3.0 (±0.8) ×10-2 ct s-1 |
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Mean XRT count rate | 1.87 (±0.25) ×10-2 ct s-1 |
RASS upper limit | 0.03 ct s-1 |
Fading? | No |
Mean flux (Observed, 0.3—10 keV) | 7.2 (±1.0) ×10-13 erg cm-2s-1 |
Peak flux (Observed, 0.3—10 keV) | 1.15 (±0.29) ×10-12 erg cm-2s-1 |
Mean rate (PSPC equivalent) | 1.97 (±0.27) ×10-2 |
Peak rate (PSPC equivalent) | 3.1 (±0.8) ×10-2 |