A new derivation of the Hubble constant from γ -ray attenuation using improved optical depths for the Fermi and CTA era

1. Domínguez, A.
2. Kirkeberg, P.Ø.
3. Wojtak, R.
4. Saldana-Lopez, A.
5. Desai, A.
6. Primack, J.R.
7. Finke, J.
8. Ajello, M.
9. Pérez-González, P.G.
10. Paliya, V.S.
11. Hartmann, D.

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DOI: 10.1093/MNRAS/STAD3425 GOOGLE SCHOLAR lock_openOpen access editor

Data source: Scopus