A new derivation of the Hubble constant from γ-ray attenuation using improved optical depths for the Fermi and CTA era by Domínguez, A, Østergaard Kirkeberg, P, Wojtak, R, Saldana-Lopez, A, Desai, A, Primack, J R, Finke, J, Ajello, M, Pérez-González, P G, Paliya, V S, Hartmann, D

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