SED of the core emission from Cen A with a one-zone SSC fit. This includes non-simultaneous observations from low to high frequencies: filled triangles (TANAMI VLBI), grey filled squares (Suzaku), open triangles (Swift-XRT/Swift -BAT), grey circles (1-year Fermi-LAT by Abdo et al. 2010a), black circles (4-year Fermi-LAT by Sahakyan et al. 2013), black filled squares (H.E.S.S. by Aharonian et al. 2009), and black open squares are archival data from Marconi et al. (2000). The solid line is our one-zone SSC model fit with some slightly different parameters than those used in Abdo et al. (2010a). For the parameters used, see Table 2.