Hostname: page-component-8448b6f56d-dnltx Total loading time: 0 Render date: 2024-04-16T06:28:51.311Z Has data issue: false hasContentIssue false
  • English
  • Français

Strong Lensing Cosmography in the Frontier Fields

Published online by Cambridge University Press:  27 October 2016

Eric Jullo ,
Ana Acebron ,
Marceau Limousin ,
Carlo Giocoli ,
Giulia Despali ,
Mario Bonamigo  and
the CATS team
Eric Jullo
Affiliation:
Aix-Marseille Université - Laboratoire d'Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille, France email: eric.jullo@lam.fr
Ana Acebron
Affiliation:
Aix-Marseille Université - Laboratoire d'Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille, France email: eric.jullo@lam.fr
Marceau Limousin
Affiliation:
Aix-Marseille Université - Laboratoire d'Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille, France email: eric.jullo@lam.fr
Carlo Giocoli
Affiliation:
Aix-Marseille Université - Laboratoire d'Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille, France email: eric.jullo@lam.fr
Giulia Despali
Affiliation:
Aix-Marseille Université - Laboratoire d'Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille, France email: eric.jullo@lam.fr
Mario Bonamigo
Affiliation:
Aix-Marseille Université - Laboratoire d'Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille, France email: eric.jullo@lam.fr
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.

The wealth of strong lensing features observed in the Frontier Fields clusters offers insights on the nature of dark energy. The large number of multiple-images systems with redshifts allows to simultaneously estimate the lens model parameters and the cosmological parameters involved in the distances calculations. In particular for the ΛCDM model, it is possible to estimate the matter density Ωm and the dark energy equations parameters wX. In this talk, I will present recent analyses of systematic errors based on Frontier Fields observed and simulated data.

Keywords

cosmological parameterscosmology: observationsgravitational lensinggalaxy clusters
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 801 - 803
Copyright
Copyright © International Astronomical Union 2016 

References

Jullo, E., Natarajan, P., Kneib, J.-P., et al., 2010, Science, 329, 924 Google Scholar
D'Aloisio, & Natarajan, 2011, MNRAS, 411, 1628 CrossRefGoogle Scholar
Jullo, E., Kneib, J.-P., Limousin, M., et al., 2007, New Journal of Phys., 9, 447 Google Scholar
Elíasdóttir, Á, Limousin, M., Richard, J., et al., 2007, eprint arXiv:0710.5636 Google Scholar
Limousin, M., Ebeling, H., Richard, J., et al., 2012, A&A, 544, 71 Google Scholar
Navarro, J. F., Frenk, C. S., & White, S. D. M., 1997 ApJ, 490, 493 Google Scholar
Giocoli, C., Tormen, G., & Sheth, R. K., 2012b, MNRAS, 422, 185 Google Scholar