H0 from cosmic chronometers and type Ia supernovae, with Gaussian processes and the novel weighted polynomial regression method
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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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
19 April 2018
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| In: |
Journal of cosmology and astroparticle physics
Year: 2018, Heft: 4, Pages: ? |
| ISSN: | 1475-7516 |
| DOI: | 10.1088/1475-7516/2018/04/051 |
| Online-Zugang: | 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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| Verfasserangaben: | 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
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