Kirk Korista
0000-0003-0944-1008
Western Michigan University
127 papers found
Refreshing results…
Hubble Space TelescopeUltraviolet Spectroscopy of 14 Low-Redshift Quasars
X-ray/ultraviolet observing campaign of the Markarian 279 active galactic nucleus outflow: a close look at the absorbing/emitting gas with Chandra-LETGS
Strong LSJ Dependence of Fluorescence Yields: Breakdown of the Configuration-Average Approximation
Importance of Configuration Interaction for Accurate Atomic Data: Fluorescence Yields of K-Shell Vacancy, Lithium-like Ions
Dielectronic recombination data for dynamic finite-density plasmas: IX. The fluorine isoelectronic sequence
Erratum: “What the Optical Recombination Lines Can Tell Us about the Broad‐Line Regions of Active Galactic Nuclei” (ApJ, 606, 749 [2004])
X‐Ray/Ultraviolet Observing Campaign of the Markarian 279 Active Galactic Nucleus Outflow: A Global‐Fitting Analysis of the Ultraviolet Absorption
X‐Ray/Ultraviolet Campaign on the Mrk 279 AGN Outflow: Constraining Inhomogeneous Absorber Models
Erratum: Dielectronic recombination data for dynamic finite-density plasmas II. The oxygen isoelectronic sequence (Astronomy and Astrophysics (2003) 412 (587-595) DOI: 10.1051/0004-6361:20031462)
Erratum: Dielectronic recombination data for dynamic finite-density plasmas IV. The carbon isoelectronic sequence (Astronomy and Astrophysics (2004) 417 (1173-1181) 10.1051/0004-6361:20034174)
The Origin of FeiiEmission in Active Galactic Nuclei
Is the slope of the intrinsic Baldwin effect constant?
What the Optical Recombination Lines Can Tell Us about the Broad‐Line Regions of Active Galactic Nuclei
Dielectronic recombination data for dynamic finite-density plasmas VII. The neon isoelectronic sequence
Dielectronic recombination data for dynamic finite-density plasmas. IV. The carbon isoelectronic sequence
Assessment of the Fluorescence and Auger DataBase Used in Plasma Modeling
Contrasting the Ultraviolet and X‐Ray OviColumn Density Inferred for the Outflow in NGC 5548
Iron Emission in z 6 QSO s
Quasar tomography: unification of echo mapping and photoionization models
Chemical Abundances in Broad Emission Line Regions: The ``Nitrogen-loud'' Quasi-Stellar Object Q0353-383
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