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Fig. 5.


Top: percentage of [NeV] emitters as a function of stellar mass for the green, red and blue galaxies. The fraction of the [NeV] emitters increases with mass in the blue cloud and decreases in the red sequence, but no statistical trend is observed in the green valley. Bottom: luminosities in the [NeV] line as a function of stellar mass. Symbols as in Fig. 4. Solid, dashed, and dotted lines show the least squares fits to the blue, green, and red [NeV] emitters, respectively. An increasing [NeV]λ3426 line luminosity is observed at larger stellar masses.

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