Fig. 9
SMF uncertainties due to cosmic variance (expressed as a fractional error: σcv/ Φ) and SED fitting (σfit/ Φ), as a function of redshift and stellar mass. We show the impact of cosmic variance on the two extreme bins 
and 
(blue and red line, respectively). For σfit we take, as an example, three redshift bins: 
(blue triangles), 
(green circles), and 
(red squares).
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