Fig. 5.
Hα-based star formation rates vs. offsets Δ MB from the local B-band Tully–Fisher relation. In contrast to field disk galaxies at z < 1 (small open squares; taken from Böhm & Ziegler 2016), the TFR offsets of the z = 1.47 (proto-)cluster galaxies (filled circles) are not correlated with star formation rate. See text for details.
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