H.E.S.S. discovery of very high energy γ -ray emission from PKS 0625-354

PKS 0625-354 (z = 0.055) was observed with the four High Energy Stereoscopic System (H.E.S.S.) telescopes in 2012 during 5.5 h. The source was detected above an energy threshold of 200 GeV at a significance level of 6.1σ. No significant variability is found in these observations. The source is well described with a power-law spectrum with photon index G = 2.84 ± 0.50 _stat ± 0.10 _syst and normalization (at E ₀ = 1.0 TeV) N ₀(E ₀)=(0.58±0.22 _stat ±0.12 _syst)×10 ^-12 TeV ^-1 cm-2 s ^-1. Multiwavelength data collected with Fermi-LAT, Swift-XRT, Swift-UVOT, ATOMand WISE are also analysed. Significant variability is observed only in the Fermi-LAT γ -ray and Swift-XRT X-ray energy bands. Having a good multiwavelength coverage from radio to very high energy, we performed a broad-band modelling from two types of emission scenarios. The results from a one zone lepto-hadronic and a multizone leptonic models are compared and discussed. On the grounds of energetics, our analysis favours a leptonic multizone model. Models associated to the X-ray variability constraint support previous results, suggesting a BL Lac nature of PKS 0625-354 with, however, a large-scale jet structure typical of a radio galaxy.