Fig. 6
Host galaxy SED of HE 2158 − 0107 within a circular aperture of 3. Open and filled symbols correspond to the SED with and without the contribution of the emission lines in the r- and i-band. The best-fit 100 Myr SSP model (blue line) and composite 100 Myr+11 Gyr SSP model (red line) taken from the Bruzual & Charlot (2003) library of spectra are shown for comparison.
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