Fig. 2
Fluxes of emission-lines in CoCoA group 2. The left graph shows CoCoA group 2 fluxes with 3σ error bars for 163 Seyfert-2s in spiral hosts. The right graph shows CoCoA group 2 fluxes for 163 Seyfert-2s in elliptical hosts, selected to match the first sample in redshift and Balmer decrement Hα/Hβ. The fluxes are in units of 10-17 erg/s/cm2.
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