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Fig. A.3.
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Stellar-mass TFR. The green points show the sample of galaxies at z ≃ 0 from McGaugh & Schombert (2015), their Table 7), and the dashed line shows the corresponding best-fitting relation. The red point shows the S0 spiral at z = 1.49 from this work with 1σ uncertainty, which is consistent with the local TFR.
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