Fig. 8 from A Multiwavelength Study of Narrow‐Line Seyfert 1 Galaxies from the Second Byurakan Survey

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A Multiwavelength Study of Narrow‐Line Seyfert 1 Galaxies from the Second Byurakan Survey

Authors: J. A. Stepanian, E. Benítez, Y. Krongold, I. Cruz-González, J. A. de Diego, V. Chavushyan, R. Mújica, D. Dultzin-Hacyan, and T. Verdugo

Stepanian et al. 2003 The Astrophysical Journal 588 746.

Provider: AAS Journals

Caption: Fig. 8.

α_ox vs. ﹩L_{\mathrm{opt}\,}﹩ for the SBS NLS1s. A weak correlation (﹩\alpha _{\mathrm{ox}\,}=0.16\mathrm{log}\,L_{\mathrm{opt}\,}-8.2﹩) can be observed for bright (﹩B\leq 17.5﹩, ﹩z\leq 0.16﹩; squares) sources. The solid line represents the best fit. Weak sources (﹩B> 17.5﹩; circles) are also shown, as well as upper limits (triangles).

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