Fig. 6.

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FVG diagram of MCG 08-11-011 between NB4250 and NB5700, NB6200, NB7320, and NB8025 (from left to right). Each data point is drawn as a thin cross in which the line length corresponds to the photometric uncertainties in the respective filters. A linear least-squares fit to the data points yields the AGN slope, plotted with the steep blue line. The cyan shaded area denotes the host color range from our multi-aperture photometry. The intersection between the AGN and the host galaxy slope gives the host contribution in the respective band within the aperture.
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