Fig. C.2

PSFs derived from the reduced R-band image of NGC 5907 (Fig. C.1). The azimuthal average is drawn as magnitude
versus radius. The left-hand set of lines used individually set background values.
The set of lines that are offset by 60′′ were all derived using the background value
1760 ADU. PSFMBH is drawn with a dotted line, together with its
error bars. The saturated-star PSFs are drawn with solid black (1) and dash-dotted
(2) lines – PSF
is the average of these two PSFs. The PSF of the remaining five bright stars are
drawn with coloured lines out to a maximum radius rmax, cf.
the legend and Table C.2.
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