Publication

Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1

Barnabe, M., Czoske, O., Koopmans, L. V. E., Treu, T. & Bolton, A. S., Aug-2011, In : Monthly Notices of the Royal Astronomical Society. 415, 3, p. 2215-2232 18 p.

Research output: Contribution to journalArticleAcademicpeer-review

APA

Barnabe, M., Czoske, O., Koopmans, L. V. E., Treu, T., & Bolton, A. S. (2011). Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1. Monthly Notices of the Royal Astronomical Society, 415(3), 2215-2232. https://doi.org/10.1111/j.1365-2966.2011.18842.x

Author

Barnabe, Matteo ; Czoske, Oliver ; Koopmans, Leon V. E. ; Treu, Tommaso ; Bolton, Adam S. / Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1. In: Monthly Notices of the Royal Astronomical Society. 2011 ; Vol. 415, No. 3. pp. 2215-2232.

Harvard

Barnabe, M, Czoske, O, Koopmans, LVE, Treu, T & Bolton, AS 2011, 'Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1', Monthly Notices of the Royal Astronomical Society, vol. 415, no. 3, pp. 2215-2232. https://doi.org/10.1111/j.1365-2966.2011.18842.x

Standard

Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1. / Barnabe, Matteo; Czoske, Oliver; Koopmans, Leon V. E.; Treu, Tommaso; Bolton, Adam S.

In: Monthly Notices of the Royal Astronomical Society, Vol. 415, No. 3, 08.2011, p. 2215-2232.

Research output: Contribution to journalArticleAcademicpeer-review

Vancouver

Barnabe M, Czoske O, Koopmans LVE, Treu T, Bolton AS. Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1. Monthly Notices of the Royal Astronomical Society. 2011 Aug;415(3):2215-2232. https://doi.org/10.1111/j.1365-2966.2011.18842.x


BibTeX

@article{612f33aaed0243f9a1b0829c95fcf7be,
title = "Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1",
abstract = "We combine in a self-consistent way the constraints from both gravitational lensing and stellar kinematics to perform a detailed investigation of the internal mass distribution, amount of dark matter, and dynamical structure of the 16 early-type lens galaxies from the Sloan Lens ACS Survey (SLACS Survey), at z = 0.08-0.33, for which both Hubble Space Telescope/Advanced camera for Surveys and NICMOS high-resolution imaging and Very Large Telescope VI-MOS integral-field spectroscopy are available. Based on this data set, we analyse the inner regions of the galaxies, that is, typically within one (three-dimensional) effective radius r(e), under the assumption of axial symmetry and by constructing dynamical models supported by two-integral stellar distribution functions. For all systems, the total mass density distribution is found to be well approximated by a simple power law rho(tot) proportional to m(-gamma)' (with m being the ellipsoidal radius): this profile is on average slightly super-isothermal, with a logarithmic slope = 2.074(-0.041)(+0.043) (errors indicate the 68 per cent confidence interval) and an intrinsic scatter sigma(gamma)' = 0.144-(+0.055)(0.014), and is fairly round, with an average axial ratio = 0.77 +/- 0.04. The lower limit for the dark matter fraction (f(DM)) inside r(e) ranges, in individual systems, from nearly zero to almost a half, with a median value of 12 per cent. By including stellar masses derived from stellar population synthesis models with a Salpeter initial mass function (IMF), we obtain an average f(DM) = 31 per cent, and the corresponding stellar profiles are physically acceptable, with the exception of two cases where they only marginally exceed the total mass profile. f(DM) rises to 61 per cent if, instead, a Chabrier IMF is assumed. For both IMFs, the dark matter fraction increases with the total mass of the galaxy (correlation significant at the 3 sigma level). Based on the intrinsic angular momentum parameter calculated from our models, we find that the galaxies can be divided into two dynamically distinct groups, which are shown to correspond to the usual classes of the (observationally defined) slow and fast rotators. Overall, the SLACS systems are structurally and dynamically very similar to their nearby counterparts, indicating that the inner regions of early-type galaxies have undergone little, if any, evolution since redshift z approximate to 0.35.",
keywords = "gravitational lensing: strong, galaxies: elliptical and lenticular, cD, galaxies: kinematics and dynamics, galaxies: structure, DARK-MATTER HALOS, DIGITAL SKY SURVEY, ELLIPTIC GALAXIES, ACS SURVEY, GRAVITATIONAL LENS, FUNDAMENTAL PLANE, INTERNAL STRUCTURE, SAURON PROJECT, X-RAY, VELOCITY PROFILES",
author = "Matteo Barnabe and Oliver Czoske and Koopmans, {Leon V. E.} and Tommaso Treu and Bolton, {Adam S.}",
year = "2011",
month = "8",
doi = "10.1111/j.1365-2966.2011.18842.x",
language = "English",
volume = "415",
pages = "2215--2232",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "Oxford University Press",
number = "3",

}

RIS

TY - JOUR

T1 - Two-dimensional kinematics of SLACS lenses - III. Mass structure and dynamics of early-type lens galaxies beyond z similar or equal to 0.1

AU - Barnabe, Matteo

AU - Czoske, Oliver

AU - Koopmans, Leon V. E.

AU - Treu, Tommaso

AU - Bolton, Adam S.

PY - 2011/8

Y1 - 2011/8

N2 - We combine in a self-consistent way the constraints from both gravitational lensing and stellar kinematics to perform a detailed investigation of the internal mass distribution, amount of dark matter, and dynamical structure of the 16 early-type lens galaxies from the Sloan Lens ACS Survey (SLACS Survey), at z = 0.08-0.33, for which both Hubble Space Telescope/Advanced camera for Surveys and NICMOS high-resolution imaging and Very Large Telescope VI-MOS integral-field spectroscopy are available. Based on this data set, we analyse the inner regions of the galaxies, that is, typically within one (three-dimensional) effective radius r(e), under the assumption of axial symmetry and by constructing dynamical models supported by two-integral stellar distribution functions. For all systems, the total mass density distribution is found to be well approximated by a simple power law rho(tot) proportional to m(-gamma)' (with m being the ellipsoidal radius): this profile is on average slightly super-isothermal, with a logarithmic slope = 2.074(-0.041)(+0.043) (errors indicate the 68 per cent confidence interval) and an intrinsic scatter sigma(gamma)' = 0.144-(+0.055)(0.014), and is fairly round, with an average axial ratio = 0.77 +/- 0.04. The lower limit for the dark matter fraction (f(DM)) inside r(e) ranges, in individual systems, from nearly zero to almost a half, with a median value of 12 per cent. By including stellar masses derived from stellar population synthesis models with a Salpeter initial mass function (IMF), we obtain an average f(DM) = 31 per cent, and the corresponding stellar profiles are physically acceptable, with the exception of two cases where they only marginally exceed the total mass profile. f(DM) rises to 61 per cent if, instead, a Chabrier IMF is assumed. For both IMFs, the dark matter fraction increases with the total mass of the galaxy (correlation significant at the 3 sigma level). Based on the intrinsic angular momentum parameter calculated from our models, we find that the galaxies can be divided into two dynamically distinct groups, which are shown to correspond to the usual classes of the (observationally defined) slow and fast rotators. Overall, the SLACS systems are structurally and dynamically very similar to their nearby counterparts, indicating that the inner regions of early-type galaxies have undergone little, if any, evolution since redshift z approximate to 0.35.

AB - We combine in a self-consistent way the constraints from both gravitational lensing and stellar kinematics to perform a detailed investigation of the internal mass distribution, amount of dark matter, and dynamical structure of the 16 early-type lens galaxies from the Sloan Lens ACS Survey (SLACS Survey), at z = 0.08-0.33, for which both Hubble Space Telescope/Advanced camera for Surveys and NICMOS high-resolution imaging and Very Large Telescope VI-MOS integral-field spectroscopy are available. Based on this data set, we analyse the inner regions of the galaxies, that is, typically within one (three-dimensional) effective radius r(e), under the assumption of axial symmetry and by constructing dynamical models supported by two-integral stellar distribution functions. For all systems, the total mass density distribution is found to be well approximated by a simple power law rho(tot) proportional to m(-gamma)' (with m being the ellipsoidal radius): this profile is on average slightly super-isothermal, with a logarithmic slope = 2.074(-0.041)(+0.043) (errors indicate the 68 per cent confidence interval) and an intrinsic scatter sigma(gamma)' = 0.144-(+0.055)(0.014), and is fairly round, with an average axial ratio = 0.77 +/- 0.04. The lower limit for the dark matter fraction (f(DM)) inside r(e) ranges, in individual systems, from nearly zero to almost a half, with a median value of 12 per cent. By including stellar masses derived from stellar population synthesis models with a Salpeter initial mass function (IMF), we obtain an average f(DM) = 31 per cent, and the corresponding stellar profiles are physically acceptable, with the exception of two cases where they only marginally exceed the total mass profile. f(DM) rises to 61 per cent if, instead, a Chabrier IMF is assumed. For both IMFs, the dark matter fraction increases with the total mass of the galaxy (correlation significant at the 3 sigma level). Based on the intrinsic angular momentum parameter calculated from our models, we find that the galaxies can be divided into two dynamically distinct groups, which are shown to correspond to the usual classes of the (observationally defined) slow and fast rotators. Overall, the SLACS systems are structurally and dynamically very similar to their nearby counterparts, indicating that the inner regions of early-type galaxies have undergone little, if any, evolution since redshift z approximate to 0.35.

KW - gravitational lensing: strong

KW - galaxies: elliptical and lenticular, cD

KW - galaxies: kinematics and dynamics

KW - galaxies: structure

KW - DARK-MATTER HALOS

KW - DIGITAL SKY SURVEY

KW - ELLIPTIC GALAXIES

KW - ACS SURVEY

KW - GRAVITATIONAL LENS

KW - FUNDAMENTAL PLANE

KW - INTERNAL STRUCTURE

KW - SAURON PROJECT

KW - X-RAY

KW - VELOCITY PROFILES

UR - http://adsabs.harvard.edu/abs/2011MNRAS.415.2215B

U2 - 10.1111/j.1365-2966.2011.18842.x

DO - 10.1111/j.1365-2966.2011.18842.x

M3 - Article

VL - 415

SP - 2215

EP - 2232

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 3

ER -

ID: 5389433