Fig. 5
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IMB SFDs: (a) cubic polynomial fit adopted for the asteroids’ SFD. The Poisson error is the square root of the asteroid count in each interval, and the range of error bars is the reciprocal of the Poisson error; (b) same cubic polynomial in (a) but with its slope b plotted as a function of H. The error bars of b are determined by Monte Carlo methods.
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