Fig. 2.
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Trends of fractions of flux collected in fiber as a function of redshift for three broad morphological classes: ETGs (left panel), spirals (central panel), and late-type and irregular galaxies (right panel). The colored points (shaded gray areas) represent the median (16th–84th percentile range) fractions relative to the footprint (see Sect. 2.3). The vertical arrows point to the median fractions relative to the growth-curve (GC) integrated flux (i.e., the footprint fraction times the fiber fraction relative to the footprint). The dashed lines indicate the 16th and 84th percentiles for the fraction relative to the total GC flux.
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