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Fig. 13


Observed LF compared to previous surveys estimates (in their closest redshift bin). The number above each LF point gives the exact number of galaxies used. The arrows going downwards correspond to measurements with an error consistent with 0. The Schechter functions fits are shown as magenta dashes. The last panel shows the evolution of the [Oii] LF from redshift 0.17 to 1.44 using the fits. The trend is that with increasing redshift there are increasing numbers of bright [Oii] emitters and the faint end slope gets steeper.

This figure is made of several images, please see below:

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