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Tommaso Treu

Researcher at University of California, Los Angeles

Publications -  796
Citations -  56051

Tommaso Treu is an academic researcher from University of California, Los Angeles. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 126, co-authored 715 publications receiving 49090 citations. Previous affiliations of Tommaso Treu include Space Telescope Science Institute & University of California.

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

TL;DR: In this paper, the authors investigate the cosmic evolution of the internal structure of massive early-type galaxies over half of the age of the universe and 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.
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The sl2s galaxy-scale lens sample. iii. lens models, surface photometry, and stellar masses for the final sample

TL;DR: In this paper, the authors used HST images and Canada-France-Hawaii Telescope (CFHT) near-infrared ground-based images for the final sample of 56 candidate galaxy-scale lenses uncovered in the CFHT Legacy Survey as part of the Strong Lensing in the Legacy Survey project.
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The properties of field elliptical galaxies at intermediate redshift – III. The Fundamental Plane and the evolution of stellar populations from z≈0.4 to z=0

TL;DR: In this paper, a sample of 25 field early-type galaxies, in the redshift range z≈0.1-0.5, selected on the basis of colours and morphology from the Medium Deep Survey (MDS) of the Hubble Space Telescope (HST), was used to study the evolution of the Fundamental Plane (FP) with redshift.
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The Stellar Velocity Dispersion of the Lens Galaxy in MG 2016+112 at z = 1.004*

TL;DR: In this article, the stellar velocity dispersion of the early-type lens galaxy D in the system MG 2016+112 (z = 1.004), determined from a spectrum obtained with the Echelle Spectrograph and Imager on the W. M. Keck II Telescope, as part of the Lenses Structure and Dynamics Survey, was presented.