Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 3(420), p. 1959-1976
DOI: 10.1111/j.1365-2966.2011.20012.x
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We present dynamical scaling relations for a homogeneous and representative sample of ~500 massive galaxies, selected only by stellar mass (>10^10 Msun) and redshift (0.025