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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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Amuse-virgo. iii. mid-infrared photometry of early-type galaxies and limits on obscured nuclear emission

TL;DR: In this article, a census of low-level nuclear activity in Virgo Cluster early-type galaxies was conducted by searching for obscured emission using Spitzer Space Telescope mid-infrared (MIR) imaging at 24 µm.
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Massive elliptical galaxies at $z \sim 0.2$ are well described by stars and a Navarro-Frenk-White dark matter halo

TL;DR: In this paper, the authors investigate the internal structure of elliptical galaxies at the expense of a joint lensing-dynamics analysis, and find that the distribution of the lensing only logarithmic slopes has a median value of 0.2.
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Modelling the AGN broad-line region using single-epoch spectra − II. Nearby AGNs

TL;DR: In this paper, the authors explore a new version of a Bayesian inference, physical model of the broad line region (BLR) which uses an individual spectrum and prior information on the BLR size from the radius-luminosity relation, to model the AGN BLR geometry and dynamics.
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Improving $z\sim7-11$ Galaxy Property Estimates with JWST/NIRCam Medium-Band Photometry

TL;DR: In this paper, the authors show that adding NIRCam images through a strategically chosen medium-band filter to common wide-band filters sets adopted by ERS and GTO programs delivers tighter constraints on these galactic properties.
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Rcs2 j232727.6-020437: an efficient cosmic telescope at z = 0:6986

TL;DR: In this article, a detailed gravitational lens model of the galaxy cluster RCS2 J232727.6-020437 was presented, where the authors identify a strong emission line in the spectrum of one multiple image, likely confirming the redshift of that system to 2.083.