Fig. 1
Four histograms of residuals comparing actual data against the model given by Eq. (1) of all sparse lightcurves belonging to the following observatories: 689 USNO, 691 Steward Observatory, 703 Catalina Sky Survey and E12 Siding Spring Survey. Number of bins is ~
, where N is the total number of sparse lightcurves used for histogram construction.
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