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The BOSS Emission-Line Lens Survey. II. Investigating mass-density profile evolution in the SLACS+BELLS strong gravitational lens sample

Bolton, Adam S.; Brownstein, Joel R.; Kochanek, Christopher S.; Shu, Yiping; Schlegel, David J.; Eisenstein, Daniel J.; Wake, David A.; Connolly, Natalia; Maraston, Claudia; Arneson, Ryan A. and Weaver, Benjamin A. (2012). The BOSS Emission-Line Lens Survey. II. Investigating mass-density profile evolution in the SLACS+BELLS strong gravitational lens sample. The Astrophysical Journal, 757(1), article no. 82.

DOI (Digital Object Identifier) Link: https://doi.org/10.1088/0004-637X/757/1/82
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Abstract

We present an analysis of the evolution of the central mass-density profile of massive elliptical galaxies from the SLACS and BELLS strong gravitational lens samples over the redshift interval ɀ ≈ 0.1-0.6, based on the combination of strong-lensing aperture mass and stellar velocity-dispersion constraints. We find a significant trend toward steeper mass profiles (parameterized by the power-law density model with ρ α r–γ) at later cosmic times, with magnitude d <γ> /dɀ = –0.60 ± 0.15. We show that the combined lens-galaxy sample is consistent with a non-evolving distribution of stellar velocity dispersions. Considering possible additional dependence of <γ> on lens-galaxy stellar mass, effective radius, and Sérsic index, we find marginal evidence for shallower mass profiles at higher masses and larger sizes, but with a significance that is subdominant to the redshift dependence. Using the results of published Monte Carlo simulations of spectroscopic lens surveys, we verify that our mass-profile evolution result cannot be explained by lensing selection biases as a function of redshift. Interpreted as a true evolutionary signal, our result suggests that major dry mergers involving off-axis trajectories play a significant role in the evolution of the average mass-density structure of massive early-type galaxies over the past 6 Gyr. We also consider an alternative non-evolutionary hypothesis based on variations in the strong-lensing measurement aperture with redshift, which would imply the detection of an "inflection zone" marking the transition between the baryon-dominated and dark-matter halo-dominated regions of the lens galaxies. Further observations of the combined SLACS+BELLS sample can constrain this picture more precisely, and enable a more detailed investigation of the multivariate dependences of galaxy mass structure across cosmic time.

Item Type: Journal Item
Copyright Holders: 2012 The American Astronomical Society
ISSN: 1538-4357
Keywords: elliptical galaxies; lenticular galaxies; cD; galactic evolution; galactic structure; gravitational lensing
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 38275
Depositing User: Astrid Peterkin
Date Deposited: 17 Sep 2013 15:21
Last Modified: 07 Dec 2018 10:18
URI: http://oro.open.ac.uk/id/eprint/38275
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