Reducing the Uncertainty on the Hubble Constant up to 35% with an Improved Statistical Analysis: Different Best-fit Likelihoods for Type Ia Supernovae, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts
Maria Giovanna Dainotti(University of Salerno), N. Fraija(Universidad Nacional Autónoma de México), Kazunari Iwasaki(The Graduate University for Advanced Studies, SOKENDAI), Giada Bargiacchi(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati), Aleksander Łukasz Lenart(Jagiellonian University), Bing Zhang(Xiamen University), Salvatore Capozzıello(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), Małgorzata Bogdan(Lund University)
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