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Tucker Jones

Researcher at University of California, Davis

Publications -  88
Citations -  3300

Tucker Jones is an academic researcher from University of California, Davis. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 29, co-authored 61 publications receiving 2864 citations. Previous affiliations of Tucker Jones include University of California, Santa Barbara & University of Hawaii.

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The Mass-Metallicity Relation at z ≃ 8: Direct-method Metallicity Constraints and Near-future Prospects

TL;DR: In this article, Jones et al. estimate gas-phase oxygen abundances in five galaxies at z = 7.1-9.1 using the direct Te method and show that the typical abundances are 7.9 (∼0.2 times the solar value) and an evolution of 0.9 ± 0.5 dex in oxygen abundance at fixed stellar mass from z ≃ 8 to 0.2
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Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at $z$$\sim$2

TL;DR: In this paper, the first sub-kiloparsec spatial resolution measurements of strongly inverted gas-phase metallicity gradients in two dwarf galaxies at 2.1 and 2.5 kpc were reported.
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Absorption Line Spectroscopy of Gravitationally-Lensed Galaxies: Further Constraints on the Escape Fraction of Ionizing Photons at High Redshift

TL;DR: In this paper, the authors used the covering fraction of low-ionization gas, measured via deep absorption line spectroscopy, as a proxy to estimate the fraction of ionizing photons escaping from high-redshift star-forming galaxies.
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HST Grism Observations of a Gravitationally Lensed Redshift 10 Galaxy

TL;DR: In this article, deep spectroscopic observations of a Lyman-break galaxy candidate (hereafter MACS1149-JD) at the WFC3/IR grisms were taken at 4 distinct position angles, totaling 34 orbits with the G141 grism.
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Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation

TL;DR: Jones et al. as discussed by the authors used the Keck/ESI echellete spectra of nine gravitationally lensed z ≃ 2-3 star-forming galaxies, probing a range of absorption transitions.