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H0 from cosmic chronometers and type Ia supernovae, with Gaussian processes and the novel weighted polynomial regression method

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In this paper we present new constraints on the Hubble parameter H 0 using: (i) the available data on H ( z ) obtained from cosmic chronometers (CCH); (ii) the Hubble rate data points extracted from the supernovae of Type Ia (SnIa) of the Pantheon compilation and the Hubble Space Telescope (HST) CAN...

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Main Authors: Gómez-Valent, Adrià (Author) , Amendola, Luca (Author)
Format: Article (Journal)
Language:English
Published: 19 April 2018
In: Journal of cosmology and astroparticle physics
Year: 2018, Issue: 4, Pages: ?
ISSN:1475-7516
DOI:10.1088/1475-7516/2018/04/051
Online Access:Verlag, Volltext: http://dx.doi.org/10.1088/1475-7516/2018/04/051
Verlag, Volltext: http://stacks.iop.org/1475-7516/2018/i=04/a=051
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Author Notes:Adrià Gómez-Valent and Luca Amendola
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H0 from cosmic chronometers and type Ia supernovae, with Gaussian processes and the novel weighted polynomial regression method by Gómez-Valent, Adrià (Author) , Amendola, Luca (Author) ,


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