Fig. D.1.
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The effect of over-subtracting Lyα on the fitted halo scale lengths. Galaxies marked with a vertical stripe are excluded from the sample due to low signal-to-noise in the halo (see Sec. 4.1). Crosses show the worst case assumption of all subtracted background flux being Lyα, and hexagons show the ratios when assuming 10% of the background being Lyα.
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