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Fig. B.2


Location of the candidate galaxies on the fundamental plane using Sersic fit parameters. The candidates are indicated by black stars. The galaxies belonging to the Ta10 sample are represented using filled green triangles, and the Tr09 sample is marked by filled cyan diamonds. The starting point of our investigation, b19, is indicated by a filled grey square. The magenta dotted lines show the limiting physical radius used in the sample sample selection. The black dashed lines are the fundamental plane fits from Appendix A with their corresponding 3σ confidence intervals shown as red solid lines. The fit appears to be slightly offset owing to the volume weights used to correct the Malmquist bias in the fitting process.

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