Fig. 1

derived in this work as a function of
. Empty squares are data with a K Johnson photometry, while filled squares are those with a Ks photometry.The third-order SBCR for early-type dwarfs is shown by the red solid line. The gray area denotes the RMS of the relation. The bottom panel presents the residual in units of the RMS of the relation. See Sect. 4 for a description of the fitting strategy.
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