RA/Dec (J2000) = 01h 21m 28.39s, -00° 39′ 14.7″ +/- 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Source 1 has been manually confirmed as the GRB afterglow so these products are no longer updated.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 |
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We expect ~9.94×10-5 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 | 1.5 (±0.3) ×10-2 ct s-1 |
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Mean XRT count rate | 1.25 (±0.14) ×10-2 ct s-1 |
RASS upper limit | 0.03 ct s-1 |
Fading? | Yes |
Mean flux (Observed, 0.3—10 keV) | 3.2 (±0.4) ×10-13 erg cm-2s-1 |
Peak flux (Observed, 0.3—10 keV) | 3.9 (±0.8) ×10-13 erg cm-2s-1 |
Mean rate (PSPC equivalent) | 1.43 (±0.17) ×10-2 |
Peak rate (PSPC equivalent) | 1.7 (±0.4) ×10-2 |