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Fig. A.2.

image

Further comparison of our spectra (black) with literature (red) spectra from Jones et al. (2009) for some of the galaxies in common between both samples (top panel) and from Cesetti et al. (2009) for our bonafide ellipticals and their average spectrum of ellipticals. The literature spectra were always scaled to match the median flux level of our spectra.

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