Fig. 16.
Galaxy templates used in photometric redshift estimations. Upper panel: basic set of Hubble types E/S0, Sbc, Scd, and Irr from Coleman et al. (1980), lower panel: collection of star-forming galaxy templates from the Kinney et al. (1996) Atlas. Their measured UV slopes, β (2200–3100 Å), are also given. In both cases the continuum was extrapolated in UV and IR as explained in Arnouts et al. (1999).
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