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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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Proceedings ArticleDOI

Liger at Keck Observatory: image detector and IFS pick-off mirror assembly

TL;DR: Liger as mentioned in this paper is a next-generation near-infrared imager and integral field spectrograph (IFS) planned for the W.M. Keck Observatory, which is designed to take advantage of improved adaptive optics from the Keck All-Sky Precision Adaptive Optics (KAPA) upgrade currently underway.
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A Preview of JWST Metallicity Studies at Cosmic Noon: The First Detection of Auroral [O ii] Emission at High Redshift

TL;DR: In this paper , an ultradeep Keck/MOSFIRE rest-optical spectra of two star-forming galaxies at z = 2.18 in the COSMOS field with bright emission lines, representing more than 20 hr of total integration.
Proceedings ArticleDOI

Innovations and advances in instrumentation at the W. M. Keck Observatory, vol. II

TL;DR: The W. M. Keck Observatory (WMKO) as discussed by the authors summarizes the performance of recently commissioned infrastructure projects, technology upgrades, and new additions to the suite of observatory instrumentation.

A strong He II $\lambda$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?

TL;DR: In this paper , the authors reported the discovery of a sub-L ∗ galaxy at z spec = 8 . 1623 + 0 . 0007 − 0. 0008 , dubbed RXJ2129-z8HeII, via the detection of a series of strong rest-frame UV / optical nebular emission lines and the clear Lyman break.
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Disentangling the Physical Origin of Emission Line Ratio Offsets at High Redshift with Spatially Resolved Spectroscopy

TL;DR: In this paper, the authors present spatially resolved Hubble Space Telescope grism spectroscopy of 15 galaxies at $z\sim 0.8$ drawn from the DEEP2 survey.