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Fig. 10.

Fig. 10. Refer to the following caption and surrounding text.

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Distribution of the fraction of galaxy types by star formation or quenching status presented for galaxies within filaments (FF) and fields at z = 0, with stellar mass controlled. Only massive galaxies that fell into filaments more than 9 Gyr ago are included. Populations are categorised into star-forming, rejuvenated, fast-quenched, and slow-quenched based on the evolution of their sSFR.

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