2011ApJ...738...41U


C.D.S. - SIMBAD4 rel 1.7 - 2020.06.02CEST11:33:24

2011ApJ...738...41U - Astrophys. J., 738, 41 (2011/September-1)

A precise cluster mass profile averaged from the highest-quality lensing data.

UMETSU K., BROADHURST T., ZITRIN A., MEDEZINSKI E., COE D. and POSTMAN M.

Abstract (from CDS):

We outline our methods for obtaining high-precision mass profiles, combining independent weak-lensing distortion, magnification, and strong-lensing measurements. For massive clusters, the strong- and weak-lensing regimes contribute equal logarithmic coverage of the radial profile. The utility of high-quality data is limited by the cosmic noise from large-scale structure along the line of sight. This noise is overcome when stacking clusters, as too are the effects of cluster asphericity and substructure, permitting a stringent test of theoretical models. We derive a mean radial mass profile of four similar mass clusters of high-quality Hubble Space Telescope and Subaru images, in the range R = 40-2800 kpc h–1, where the inner radial boundary is sufficiently large to avoid smoothing from miscentering effects. The stacked mass profile is detected at 58σ significance over the entire radial range, with the contribution from the cosmic noise included. We show that the projected mass profile has a continuously steepening gradient out to beyond the virial radius, in remarkably good agreement with the standard Navarro-Frenk-White form predicted for the family of cold dark matter (CDM) dominated halos in gravitational equilibrium. The central slope is constrained to lie in the range, -dln ρ/dln r = 0.89+0.27_- 0.39_. The mean concentration is cvir= 7.68+0.42 _- 0.40_(at Mvir= 1.54+0.11_- 0.10_x1015 Mh–1), which is high for relaxed, high-mass clusters, but consistent with ΛCDM when a sizable projection bias estimated from N-body simulations is considered. This possible tension will be more definitively explored with new cluster surveys, such as CLASH, LoCuSS, Subaru Hyper Suprime-Cam, and XXM-XXL, to construct the cvir-Mvir relation over a wider mass range.

Abstract Copyright:

Journal keyword(s): cosmology: observations - dark matter - galaxies: clusters: general - gravitational lensing: strong - gravitational lensing: weak

Status at CDS:  

Simbad objects: 7

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Number of rows : 7

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 ZwCl 0024+1652 ClG 00 26 36.0 +17 08 36     18.35     ~ 603 1
2 ACO 370 ClG 02 39 50.5 -01 35 08           ~ 636 0
3 ACO 383 ClG 02 48 06.9 -03 29 32           ~ 296 0
4 ACO 1689 ClG 13 11 29.5 -01 20 28           ~ 1017 0
5 ACO 1703 ClG 13 15 05.2 +51 49 02           ~ 120 0
6 ClG J1347-1145 ClG 13 47 33.5 -11 45 42           ~ 463 0
7 ZwCl 1358+6245 ClG 13 59 54.3 +62 30 36     18.5     ~ 348 0

    Equat.    Gal    SGal    Ecl

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2020.06.02-11:33:24

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