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The Hubble Constant from the HST Key Project on the Extragalactic Distance Scale

Laura Ferrarese·Brad Gibson·Daniel Kelson·Shoko Sakai·Jeremy Mould·Wendy Freedman·Robert Kennicutt·Holland Ford·John Graham·John Huchra·Shaun Hughes·Garth Illingworth·Lucas Macri·Barry Madore·Kim Sebo·N. A. Silbermann·Peter Stetson
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Abstract

The final efforts of the HST Key Project on the Extragalactic Distance Scale are presented. Four distance indicators, the Surface Brightness Fluctuation method, the Fundamental Plane for early-type galaxies, the Tully-Fisher relation and the Type Ia Supernovae, are calibrated using Cepheid distances to galaxies within 25 Mpc. The calibration is then applied to distant samples reaching cz~10000 km/s and (in the case of SNIa) beyond. By combining the constraints imposed on the Hubble constant by the four distance indicators, we obtain H0 = 71+/-6 km/s/Mpc.

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Laura Ferrarese, Brad Gibson, Daniel Kelson, Shoko Sakai, Jeremy Mould, Wendy Freedman, Robert Kennicutt, Holland Ford, John Graham, John Huchra, Shaun Hughes, Garth Illingworth, Lucas Macri, Barry Madore, Kim Sebo, N. A. Silbermann, Peter Stetson. 1999-09-07. The Hubble Constant from the HST Key Project on the Extragalactic Distance Scale. https://arxiv.org/abs/astro-ph/9909134

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