DOI: 10.1051/0004-6361/200911963
The mass profile of early-type galaxies in overdense environments: the case of the double source-plane gravitational lens SL2SJ02176-0513
H. Tu1, 2, 3, R. Gavazzi2, 3, 4, M. Limousin5, 6, 7, R. Cabanac5, P. J. Marshall4, B. Fort2, 3, T. Treu4, R. Péllo8, E. Jullo6, 9, J.-P. Kneib6, 10, and J.-F. Sygnet2, 31 Physics Department & Shanghai Key Lab for Astrophysics, Shanghai Normal University, 100 Guilin Road, Shanghai 200234, PR China
e-mail: tuhong@shnu.edu.cn
2 CNRS, UMR7095, Institut d'Astrophysique de Paris, 98bis Bd Arago, 75014, Paris, France
3 UPMC Univ. Paris 6, UMR7095, Institut d'Astrophysique de Paris, 98bis Bd Arago, 75014, Paris, France
4 Department of Physics, University of California, Santa Barbara, CA 93106, USA
5 Laboratoire d'Astrophysique de Toulouse-Tarbes, Université de Toulouse, CNRS, 57 avenue d'Azereix, 65000 Tarbes, France
6 OAMP, Laboratoire d'Astrophysique de Marseille - UMR 6110, Traverse du siphon, 13012 Marseille, France
7 Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, 2100 Copenhagen, Denmark
8 Laboratoire d'Astrophysique de Toulouse-Tarbes, CNRS-UMR 5572, and Univ. Paul Sabatier, 31400 Toulouse, France
9 European Southern Observatory, Alonso de Cordoba, Santiago, Chile
10 Department of Astronomy, California Institute of Technology, 105-24, Pasadena, CA91125, USA
Received 27 February 2009 / Accepted 13 April 2009
Abstract
Context. The Strong Lensing Legacy Survey (SL2S) provides a sample of the
strong lensing events associated with massive distant galaxies, some
of which lie in the outskirts of galaxy groups and clusters.
Aims. We investigate the internal structure of early-type galaxies in
overdense environments, where tidal forces are expected to alter
dark matter haloes of infalling galaxies.
Methods. SL2SJ02176-0513 is a remarkable lens for the presence of two multiply-imaged
systems at different redshifts lensed by a foreground massive galaxy
at
= 0.656: a bright cusp arc at
= 1.847 and an additional
double-image system at an estimated redshift of
~ 2.9 based
on photometry and lensing geometry. The system is located about
400 kpc away from the centre of a massive group of galaxies. Mass
estimates for the group are available from X-ray observations and
satellite kinematics. Multicolour photometry provides an estimate of
the stellar mass of the main lens galaxy. The lensing galaxy is
modelled with two components (stars and dark matter), and we include
the perturbing effect of the group environment and all available
constraints.
Results. We find that classic lensing degeneracies, e.g. between external
convergence and mass density slope, are significantly reduced with
respect to standard systems and infer tight constraints on the mass
density profile: (i) the dark matter content of the main lens galaxy
is in line with that of typical galaxies
; (ii) the required mass
associated with the dark matter halo of the nearby group is
consistent with X-ray
;
(iii) accounting for the group contribution in the form of an external
convergence, the slope of the mass density profile of the main lens
galaxy alone is found to be
,
consistent with the isothermal (
= -1) slope.
Conclusions. We demonstrate that multiple source plane systems together with good
ancillary dataset can be used to disentangle local and environmental
effects.
Key words: gravitational lensing -- Galaxy: general -- dark matter
© ESO 2009

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