As Fig. 11 for the hyperluminous IR galaxy IRAS 10214+4724 with data from NED, Spitzer IRS (Hernán-Caballero & Hatziminaoglou 2011), and MIPS, IRAC and Herschel by Efstathiou et al. (2013). A fit using pure AGN models are shown with (dashed) and without (dotted) clumps. Model parameters are given in Table 3.
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