Spectral energy distribution of PKS2005-489 during this multi-wavelength campaign with simultaneous observations by H.E.S.S., Fermi/LAT, RXTE, Swift and ATOM (black symbols) using the time range shown in Fig. 1. The spectra shown here are corrected for Galactic extinction, N_H absorption, and EBL absorption. The size of the symbols for the optical data represent the flux range measured. The deabsorbed X-ray and TeV spectra of PKS 2005-489 in 2004 (H.E.S.S. Collaboration 2010), as well as historical IR and radio observations are shown in grey. The black curves represent a one zone SSC model as described in the text.