Fig. 11.

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Star formation rate averaged over the past 100 Myr (SFR100) versus stellar mass for our final 52 TDE hosts split into two redshift bins (0.0 ≤ z < 0.2 and 0.2 ≤ z < 0.8). The pink background shows the volume-limited SDSS comparison sample described with SFR measurement. The solid black line marks the redshift-dependent star-forming main sequence from Popesso et al. (2023).
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