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Title: The SL2S galaxy-scale lens sample. V. dark matter halos and stellar IMF of massive early-type galaxies out to redshift 0.8

Journal Article · · The Astrophysical Journal (Online)
 [1];  [2];  [3];  [4];  [5];  [6];  [7]
  1. Univ. of California, Santa Barbara, CA (United States). Physics Dept.
  2. Univ. of California, Santa Barbara, CA (United States). Physics Dept.; Univ. of California, Los Angeles, CA (United States). Dept. of Physics and Astronomy
  3. Kavli Inst. for Particle Astrophysics and Cosmology, Stanford, CA (United States)
  4. Academia Sinica, Taipei (Taiwan). Inst. of Astronomy and Astrophysics
  5. Univ. Pierre et Marie Curie, Paris (France). Inst. of Astrophysics
  6. Univ. of Cambridge (United Kingdom). Inst. of Astronomy
  7. Bologna Univ. (Italy). Dept. of Physics and Astronomy

Here, we investigate the cosmic evolution of the internal structure of massive early-type galaxies over half of the age of the universe. We also perform a joint lensing and stellar dynamics analysis of a sample of 81 strong lenses from the Strong Lensing Legacy Survey and Sloan ACS Lens Survey and combine the results with a hierarchical Bayesian inference method to measure the distribution of dark matter mass and stellar initial mass function (IMF) across the population of massive early-type galaxies. Lensing selection effects are taken into account. Furthermore, we found that the dark matter mass projected within the inner 5 kpc increases for increasing redshift, decreases for increasing stellar mass density, but is roughly constant along the evolutionary tracks of early-type galaxies. The average dark matter slope is consistent with that of a Navarro-Frenk-White profile, but is not well constrained. The stellar IMF normalization is close to a Salpeter IMF at log M * = 11.5 and scales strongly with increasing stellar mass. No dependence of the IMF on redshift or stellar mass density is detected. The anti-correlation between dark matter mass and stellar mass density supports the idea of mergers being more frequent in more massive dark matter halos.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1336371
Report Number(s):
SLAC-PUB-16265
Journal Information:
The Astrophysical Journal (Online), Vol. 800, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 105 works
Citation information provided by
Web of Science

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AutoLens: automated modeling of a strong lens’s light, mass, and source journal May 2018
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Calibrated, cosmological hydrodynamical simulations with variable IMFs – II. Correlations between the IMF and global galaxy properties journal October 2018
Total density profile of massive early-type galaxies in H  orizon -AGN simulation: impact of AGN feedback and comparison with observations journal December 2018
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The LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release text January 2016
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SHARP - V. Modelling gravitationally-lensed radio arcs imaged with global VLBI observations text January 2018
Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample text January 2018
LinKS: Discovering galaxy-scale strong lenses in the Kilo-Degree Survey using Convolutional Neural Networks text January 2018
The Extremely High Dark Matter Halo Concentration of the Relic Compact Elliptical Galaxy Mrk 1216 text January 2019
Survey of gravitationally-lensed objects in HSC imaging (SuGOHI). III. Statistical strong lensing constraints on the stellar IMF of CMASS galaxies text January 2019
Mapping the dark matter halo of early-type galaxy NGC 2974 through orbit-based models with combined stellar and cold gas kinematics text January 2019
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