Query : 2010A&A...519A..91F

2010A&A...519A..91F - Astronomy and Astrophysics, volume 519, A91-91 (2010/9-1)

Strong lensing in the MARENOSTRUM UNIVERSE. II. Scaling relations and optical depths.


Abstract (from CDS):

The strong lensing events that are observed in compact clusters of galaxies can, both statistically and individually, return important clues about the structural properties of the most massive structures in the Universe. Substantial work is ongoing in order to understand the degree of similarity between the lensing cluster population and the population of clusters as a whole, with members of the former being likely more massive, compact, and substructured than members of the latter. In this work we exploit synthetic clusters extracted from the McareNcostrum Ucniverse cosmological simulation in order to estimate the correlation between the strong lensing efficiency and other bulk properties of lensing clusters, such as the virial mass and the bolometric X-ray luminosity. We found that a positive correlation exist between all these quantities, with the substantial scatter being smaller for the luminosity-cross section relation. We additionally used the relation between the lensing efficiency and the virial mass in order to construct a synthetic optical depth that agrees well with the true one, while being extremely faster to be evaluated. We finally estimated what fraction of the total giant arc abundance is recovered when galaxy clusters are selected according to their dynamical activity or their X-ray luminosity. Our results show that there is a high probability for high-redshift strong lensing clusters to be substantially far away from dynamical equilibrium, and that 30-40% of the total amount of giant arcs are lost if looking only at very X-ray luminous objects.

Abstract Copyright:

Journal keyword(s): gravitational lensing: strong - galaxies: clusters: general

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
1 ClG J0224-0002 ClG 02 24 34.10 -00 02 30.9           ~ 50 1
2 ClG J1620+2929 ClG 16 20 09.4 +29 29 26           ~ 19 0
3 ClG J2156-0448 ClG 21 56 41 -04 48.1           ~ 15 0
4 ClG J2319+0038 ClG 23 19 53 +00 38.0           ~ 38 1

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