Updated atomic data allow consistent photoionization models to reproduce both optical and NIR FeII emission in IZw1 at densities 10^11-10^12 cm^-3 and near-solar metallicity, with Lyman-alpha fluorescence dominant in NIR.
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Simultaneous modeling of FeII emission in the optical and near-infrared in a prototypical Narrow-Line Seyfert 1 galaxy
Updated atomic data allow consistent photoionization models to reproduce both optical and NIR FeII emission in IZw1 at densities 10^11-10^12 cm^-3 and near-solar metallicity, with Lyman-alpha fluorescence dominant in NIR.