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Uncovering Obscured Active Galactic Nuclei in Homogeneously Selected Samples of Seyfert 2 Galaxies

  • Authors: Stephanie M. LaMassa, T. M. Heckman, A. Ptak, L. Martins, V. Wild, P. Sonnentrucker, and A. Hornschemeier

LaMassa et al. 2011 The Astrophysical Journal 729 52.

  • Provider: AAS Journals

Caption: Figure 2.

Histograms showing the distribution of obscuration diagnostic ratios ( F 2–10 keV/ F isotropic). Dark blue histogram represents the non-variable 12 μm sources, cyan reflects the X-ray variable 12 μm sources (X-ray fluxes are averaged for each source), red denotes the [O iii] sample and the gray shaded region illustrates the average value for Sy1s from (a) Heckman et al. (2005), log ( lang ) = 1.59 ± 0.49 dex, (b) Diamond-Stanic et al. (2009), log ( lang ) = 1.92 ± 0.60 dex, and (c) Gandhi et al. (2009), log ( lang F 2–10 keV/ F MIR rang) = −0.34 ±0.30 dex. The left facing arrows represent X-ray upper limits in (a)–(c) and right facing arrows illustrate the [O iv] upper limits in (b); these values are not included in the histogram.

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