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Fig. 7

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B-band TFR for the combined sample of cluster (55) and field (57) galaxies. Only high-quality objects are considered. The blue solid line indicates the best-fit inverse regression line. The blue dotted lines depict the corresponding 1σ and 3σ intervals, respectively. The green and red lines are the best-fit forward and bisector fits, respectively. Black open circles indicate the positions of the low-quality objects.

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