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Kevin N. Hainline

Researcher at University of Arizona

Publications -  85
Citations -  3197

Kevin N. Hainline is an academic researcher from University of Arizona. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 29, co-authored 49 publications receiving 2766 citations. Previous affiliations of Kevin N. Hainline include University of California, Los Angeles & Steward Health Care System.

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Journal ArticleDOI

Black Hole Variability and the Star Formation-Active Galactic Nucleus Connection: Do All Star-forming Galaxies Host an Active Galactic Nucleus?

TL;DR: In this article, the authors investigate the effect of AGN variability on the observed connection between star formation and black hole accretion in extragalactic surveys, and show that there may be a tight connection between AGN activity and SFR over galaxy evolution timescales, and that the apparent similarities in rest-frame colors, merger rates, and clustering of AGNs compared to inactive galaxies may be due primarily to AGNs variability.
Journal ArticleDOI

Black hole variability and the star formation-AGN connection: Do all star-forming galaxies host an AGN?

TL;DR: In this article, the authors investigate the effect of active galactic nucleus variability on the observed connection between star formation and black hole accretion in extragalactic surveys, and show that the apparent similarities in rest-frame colors, merger rates, and clustering of AGNs compared to "inactive" galaxies may be due primarily to AGN variability.
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REST-FRAME OPTICAL SPECTRA OF THREE STRONGLY LENSED GALAXIES AT z ~ 2

TL;DR: In this paper, Keck II NIRSPEC spectra for three recently discovered lensed galaxies: the Cosmic Horseshoe, the Clone and SDSS J090122.37+181432.3 have been measured.
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A Direct Measurement of the Linear Bias of Mid-infrared-selected Quasars at z ≈ 1 Using Cosmic Microwave Background Lensing

James E. Geach, +64 more
TL;DR: In this paper, the authors measured the cross-power spectrum of the projected mass density as traced by the convergence of the cosmic microwave background lensing field from the South Pole Telescope (SPT) and a sample of Type 1 and 2 (unobscured and obscured) quasars at 〈z〉 ~ 1 selected with the Wide-field Infrared Survey Explorer, over 2500 deg^2.
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The Kinematics of Multiple-Peaked Lyα Emission in Star-Forming Galaxies at z ~ 2-3

TL;DR: In this paper, the authors used a large spectroscopic database of UV-selected star-forming galaxies at high redshifts to study the Lyα emission-line kinematics.