Fig. 3
Spectral energy distribution of η Car for DS-I (black) and DS-II (red). H.E.S.S. points show 1σ statistical errors. The shaded regions indicate the combined statistical and systematic errors (as given in the main text and Table 3). Fermi-LAT spectra from Reitberger et al. (2015) for the full orbit (grey) and for the last periastron passage from Balbo & Walter (2017) (blue) are also shown.
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