Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-25T15:59:54.105Z Has data issue: false hasContentIssue false
  • English
  • Français

Cosmography with high-redshift probes

Published online by Cambridge University Press:  01 July 2015

Vincenzo Vitagliano
Vincenzo Vitagliano*
Affiliation:
CENTRA, Instituto Superior Técnico, Universidade de Lisboa, Av. Rovisco Pais 1, 1049 Lisboa, Portugal email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

I discuss how the cosmographic approach to the determination of cosmological parameters can be implemented with the inclusion of high-redshift data. I argue on the viability of such high-z probes for cosmographic purposes, and resume some statistical issues in finding the most reliable cosmographic truncation.

Keywords

cosmological parameterscosmology: miscellaneous
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Symposium S306: Statistical Challenges in 21st Century Cosmology , May 2014 , pp. 210 - 212
Copyright
Copyright © International Astronomical Union 2015 

References

Cattoen, C. & Visser, M., 2007 Class. Quant. Grav. 24, 5985.CrossRefGoogle Scholar
Visser, M., 2004 Class. Quant. Grav. 21, 2603.CrossRefGoogle Scholar
Vitagliano, V., Xia, J.-Q., Liberati, S. & Viel, M., 2010 JCAP 1003, 005.CrossRefGoogle Scholar
Xia, J.-Q., Vitagliano, V., Liberati, S. & Viel, M., 2012 Phys. Rev. D 85, 043520.Google Scholar