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In this proceeding, we briefly highlight the contributions to the 6th International Symposium on High Energy Gamma-Ray Astronomy that were on behalf of the H.E.S.S. Collaboration, with particular focus given to those results shown publicly for the first time at this symposium. Many of these new results were made possible by the improved capabilities of the H.E.S.S. II telescope array, namely its increased sensitivity to γ-rays and lower energy threshold. Other important results capitalized on the very large datasets accumulated by H.E.S.S. I observations over the last 12 years. Prominent highlights cover a diverse range of topics and astronomical objects: the Galactic center, pulsars, pulsar wind nebulae, shell-type supernova remnants, γ-ray binaries, unidentified sources, flat-spectrum radio quasars, blazars, gamma-ray bursts, fast radio bursts, neutrino event follow-up, and Lorentz invariance violation. [ABSTRACT FROM AUTHOR]