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A. J. Metevier

Researcher at University of California, Santa Cruz

Publications -  11
Citations -  709

A. J. Metevier is an academic researcher from University of California, Santa Cruz. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 9, co-authored 11 publications receiving 693 citations. Previous affiliations of A. J. Metevier include Sonoma State University.

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The stellar mass Tully-Fisher relation to z = 1.2 from AEGIS

TL;DR: In this paper, the authors combine newly measured rotation velocities, velocity dispersions, and stellar masses to construct stellar mass Tully-Fisher relations (M*TFRs) for 544 galaxies with strong emission lines at 0.1 < z < 1.2, with no detectable evolution of its intercept or slope with redshift.
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The Bright SHARC Survey: The Cluster Catalog

TL;DR: The Bright SHARC Survey as discussed by the authors is a large-scale search for serendipitously detected extended X-ray sources in 460 deep ROSAT PSPC pointings and has yielded 374 extended sources with a redshift range from 0.0696 to 0.83 and a luminosity range of 0.3e44 erg/s.
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Triggered or self-regulated star formation within intermediate redshift luminous infrared galaxies. i. morphologies and spectral energy distributions

TL;DR: In this paper, a set of 15 intermediate redshift (z ~ 0.8) luminous infrared (IR) galaxies (LIRGs) with the Keck Laser Guide Star (LGS) AO facility were selected from the Great Observatories Origins Deep Survey (GOODS) southern field, allowing them to combine the high spatial resolution Hubble Space Telescope optical (B, V, i, and z-bands) images with our near-infrared (K'-band) images to study the LIRG morphologies and spatially resolved spectral energy distributions (S
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Triggered or Self-Regulated Star Formation within Intermediate Redshift Luminous Infrared Galaxies (I). Morphologies and Spatially Resolved Spectral Energy Distributions

TL;DR: In this article, a set of 15 intermediate redshift luminous infrared galaxies (LIRGs) with the Keck Laser Guide Star (LGS) AO facility were selected from the GOODS-S field, allowing them to combine the high spatial resolution HST optical (B, V, i, and z-bands) images with their near-infrared (K'-band) images to study the LIRG morphologies and spatially resolved spectral energy distributions.