2007ApJ...671.1466K


Query : 2007ApJ...671.1466K

2007ApJ...671.1466K - Astrophys. J., 671, 1466-1470 (2007/December-3)

The mass of the Coma cluster from weak lensing in the Sloan Digital Sky Survey.

KUBO J.M., STEBBINS A., ANNIS J., DELL'ANTONIO I.P., LIN H., KHIABANIAN H. and FRIEMAN J.A.

Abstract (from CDS):

We present a weak-lensing analysis of the Coma Cluster using the Sloan Digital Sky Survey Data Release 5. Complete imaging of an ∼200 deg2 region is used to measure the tangential shear of this cluster. The shear is fit to a Navarro, Frenk, & White model, and we find a virial radius of r200=1.99+0.21–0.22 h–1 Mpc, which corresponds to a virial mass of M200=1.88+0.65–0.56x1015 h–1 M☉. We additionally compare our weak-lensing measurement to the virial mass derived using dynamical techniques and find that they are in agreement. This is the lowest redshift, largest angle weak-lensing measurement of an individual cluster to date.

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Journal keyword(s): Galaxies: Clusters: Individual: Name: Coma - Cosmology: Gravitational Lensing

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 4874 LIN 12 59 35.7093764280 +27 57 33.293892204 13.01 13.7 12.71 12.27 11.386 ~ 814 3
2 ACO 1656 ClG 12 59 44.40 +27 54 44.9           ~ 5141 2
3 NGC 4889 EmG 13 00 08.097 +27 58 37.29 12.93 13.0 11.30 11.652 10.906 ~ 742 1
4 ACO 3667 ClG 20 12 33.68 -56 50 26.3           ~ 676 1

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