A catalog of near-IR absolute magnitudes of Solar System small bodies

Open Access

Fig. 7

Comparison between measured and modeled magnitudes using the ${H G}_{12}^{*}$ $\[\mathrm{HG}_{12}^{*}\]$ model. Different panels show data in different filters. The continuous line indicates a running median of 21 points. Typical error bars in the y axis are shown in the lower right corner for reference.

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