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Fig. 5

image

Fractions of the break types as a function of the galaxy Hubble type in the infrared sample shown separately for low mass (left panel), and high mass bins (right panel). The galaxies are divided to low and high mass bins by the median mass of the Hubble type bins shown in Fig. 1. The error bars are calculated using binomial statistics, and denote the ± 1σ uncertainties.

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