Fig. 10.
Comparison of the NIBLES optically corrected HIMF (black dots denote the data points, and the black line the Schechter fit) and the Z03 and H11 blind HI survey HIMFs (blue and purple dots denote the data points from Z03 and H11, respectively, which have been rescaled to match the NIBLES flux scale (see text) and Hubble constant used in this paper).
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