Fig. 1

Fraction of the sky (top: |b| < 10°, bottom: |b| > 10°) covered by the BAT survey as a function of the 15–150 keV detection limiting flux for a detection threshold of 4.8 standard deviations. Different colours refer to different survey epochs. The insets show the limiting flux achieved for 50% of the sky as a function of time; the best fit is a power law consistent with t-0.5.
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