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Fig. 10

image

Ratio RW of the shorter two and longer two wavelength bands of WISE plotted against XUV. Blue crosses are objects without significant emission lines in the spectrum (spectral type 0 and 1), green open squares LEGs (spectral type 2) and red dots are HEGs (spectral type 3 and 4, see Table 4). The dashed horizontal line is the expected RW for elliptical galaxies with only an old stellar population. The magenta line is the linear regression of RW against XUV (see text).

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