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Kirk T. Korista

Researcher at Western Michigan University

Publications -  206
Citations -  17519

Kirk T. Korista is an academic researcher from Western Michigan University. The author has contributed to research in topics: Emission spectrum & Active galactic nucleus. The author has an hindex of 70, co-authored 202 publications receiving 16065 citations. Previous affiliations of Kirk T. Korista include University of Western Ontario & University of Kentucky.

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CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra

TL;DR: In this article, the authors describe version 90 (C90) of the code, paying particular attention to changes in the atomic database and numerical methods that have affected predictions since the last publicly available version, C84.
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Atomic data for astrophysics. II. New analytic fits for photoionization cross sections of atoms and ions

TL;DR: In this article, a complete set of analytic fits to the nonrelativistic photoionization cross sections for the ground states of atoms and ions of elements from H through Si, and S, Ar, Ca, and Fe were presented.
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Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. I, an 8 month campaign of monitoring NGC 5548 with IUE

J. Clavel, +56 more
TL;DR: In this paper, an 8-month campaign of monitoring NGC 5548 with IUE is described, with the goal of determining the size and structure of the broad-line region in active galactic nuclei.
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Locally Optimally Emitting Clouds and the Origin of Quasar Emission Lines

TL;DR: In this article, a large grid of photoionization models covering the widest possible range of cloud gas density and distance from the central continuum source was computed, and it was shown that for each line, only a narrow range of density and distances from the source results in maximum reprocessing efficiency, corresponding to locally optimally emitting clouds.
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Steps toward determination of the size and structure of the broad-line region in active galatic nuclei. 8: an intensive HST, IUE, and ground-based study of NGC 5548

TL;DR: In this paper, the authors presented the data and initial results from a combined Hubble Space Telescope (HST)/IUE/ground-based spectroscopic monitoring campaign on the Seyfert 1 galaxy NGC 5548 that was undertaken in order to address questions that require both higher temporal resolution and higher signal-to-noise ratios than were obtained in our previous multiwavelength monitoring of this galaxy in 1988-1989.