Abstract
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 Ω m and the dark energy equations parameters w X. In this talk, I will present recent analyses of systematic errors based on Frontier Fields observed and simulated data.
Original language | English |
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Pages (from-to) | 801-803 |
Number of pages | 3 |
Journal | Proceedings of the International Astronomical Union |
Volume | 11 |
Issue number | A29B |
DOIs | |
State | Published - 1 Jan 2015 |
Externally published | Yes |
Keywords
- cosmological parameters
- cosmology: observations
- galaxy clusters
- gravitational lensing
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science