Fig. 4.
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FIR–radio correlation for the analyzed early-type galaxies. Symbols denote the same classes of sources as in Figure 3, except for objects with only upper limit measurements in the FIR, which are marked with stars. Gray shaded area denotes the q-values consistent with the range corresponding q = 2.40 ± 2σq with σq = 0.24 (Ivison et al. 2010).
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