RA/Dec (J2000) = 11h 33m 49.30s, +40° 52′ 39.8″ +/- 4.2 (radius, 90%)
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This is the probable afterglow because:
Light curve | Spectrum |
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We expect ~4.89×10-3 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 | 3.8 (±1.2) ×10-3 ct s-1 |
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Mean XRT count rate | 3.8 (±1.2) ×10-3 ct s-1 |
RASS upper limit | 0.04 ct s-1 |
Fading? | Yes |
Mean flux (Observed, 0.3—10 keV) | 2.1 (±0.7) ×10-13 erg cm-2s-1 |
Peak flux (Observed, 0.3—10 keV) | 2.1 (±0.7) ×10-13 erg cm-2s-1 |
Mean rate (PSPC equivalent) | 10 (±3) ×10-4 |
Peak rate (PSPC equivalent) | 10 (±3) ×10-4 |