Fig. 11
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Distribution of asteroids identified in HST images by ecliptic latitude. (a) Number of identified (blue) and unidentified (orange) objects by ecliptic latitude. (b) Number density of detected asteroids with magnitudes <24.5 mag, as a function of ecliptic latitude, for the two HST instruments. The errors are the 68% (1σ) confidence limits from the Wilson (1927) binomial confidence interval.
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