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Table 1

List of previous publications (we do not claim completeness) of fundamental plane coefficients, based on the list of Magoulas et al. (2012), which is itself based on the lists of Bernardi et al. (2003c) and Colless et al. (2001).

Band a b c σdist [%] N gal Type of fit Authors
B 1.39 ± 0.14 −0.90 ± 0.09 − 20 106 2-step inverse R Djorgovski & Davis (1987)
B 1.33 ± 0.05 −0.83 ± 0.03 − 20 97 inverse R Dressler et al. (1987)
V + R 1.43 ± 0.03 −0.84 ± 0.02 −7.995 ± 0.021 21 694 inverse R Smith et al. (2001)
R 1.38 ± 0.04 −0.82 ± 0.03 − 21 352 inverse R Hudson et al. (1997)
R 1.37 ± 0.05 −0.84 ± 0.03 − 21 428 inverse R Gibbons et al. (2001)
V 1.26 ± 0.07 −0.82 ± 0.09 − 13 66 forward R Lucey et al. (1991)
V 1.14 −0.79 − 17 37 forward R Guzman et al. (1993)
r 1.24 ± 0.07 −0.82 ± 0.02 − 17 226 orthogonal R Jorgensen et al. (1996)
R 1.25 −0.87 − 19 40 orthogonal R Müller et al. (1998)
V 1.21 ± 0.05 −0.80 ± 0.01 − − − orthogonal R D’Onofrio et al. (2008)
r 1.42 ± 0.05 −0.76 ± 0.008 − 28 1430 orthogonal R La Barbera et al. (2008)
K 1.53 ± 0.04 −0.77 ± 0.01 − 29 1430 orthogonal R La Barbera et al. (2008)
R 1.35 ± 0.11 −0.81 ± 0.03 − 21 91 orthogonal R Gargiulo et al. (2009)
g 1.40 ± 0.02 −0.76 ± 0.02 −8.858 31 46 410 orthogonal R Hyde & Bernardi (2009)
r 1.43 ± 0.02 −0.79 ± 0.02 −8.898 30 46 410 orthogonal R Hyde & Bernardi (2009)
i 1.46 ± 0.02 −0.80 ± 0.02 −8.891 29 46 410 orthogonal R Hyde & Bernardi (2009)
z 1.47 ± 0.02 −0.83 ± 0.02 −9.032 29 46 410 orthogonal R Hyde & Bernardi (2009)
g 1.38 ± 0.02 −0.788 ± 0.002 −9.13 ± 0.08 29 4467 orthogonal R La Barbera et al. (2010a)
r 1.39 ± 0.02 −0.785 ± 0.002 −8.84 ± 0.06 26 4478 orthogonal R La Barbera et al. (2010a)
i 1.43 ± 0.02 −0.780 ± 0.002 −8.76 ± 0.05 − 4455 orthogonal R La Barbera et al. (2010a)
z 1.42 ± 0.02 −0.793 ± 0.002 −8.74 ± 0.07 − 4319 orthogonal R La Barbera et al. (2010a)
Y 1.47 ± 0.02 −0.785 ± 0.002 −8.53 ± 0.06 − 4404 orthogonal R La Barbera et al. (2010a)
J 1.53 ± 0.02 −0.795 ± 0.002 −8.57 ± 0.06 26 4317 orthogonal R La Barbera et al. (2010a)
H 1.56 ± 0.02 −0.795 ± 0.002 −8.42 ± 0.08 27 4376 orthogonal R La Barbera et al. (2010a)
K 1.55 ± 0.02 −0.790 ± 0.002 −8.24 ± 0.08 28 4350 orthogonal R La Barbera et al. (2010a)
K 1.53 ± 0.08 −0.79 ± 0.03 − 21 251 orthogonal R Pahre et al. (1998)
V 1.31 ± 0.13 −0.86 ± 0.10 − 14 30 orthogonal R Kelson et al. (2000)
R 1.22 ± 0.09 −0.84 ± 0.03 − 20 255 orthogonal ML Colless et al. (2001)
g 1.45 ± 0.06 −0.74 ± 0.01 −8.779 ± 0.029 25 5825 orthogonal ML Bernardi et al. (2003c)
r 1.49 ± 0.05 −0.75 ± 0.01 −8.778 ± 0.020 23 8228 orthogonal ML Bernardi et al. (2003c)
i 1.52 ± 0.04 −0.78 ± 0.01 −8.895 ± 0.021 23 8022 orthogonal ML Bernardi et al. (2003c)
z 1.51 ± 0.04 −0.77 ± 0.01 −8.707 ± 0.023 22 7914 orthogonal ML Bernardi et al. (2003c)
J 1.52 ± 0.03 −0.89 ± 0.008 − 30 8901 orthogonal ML Magoulas et al. (2012)
H 1.47 ± 0.02 −0.88 ± 0.008 − 29 8568 orthogonal ML Magoulas et al. (2012)
K 1.46 ± 0.02 −0.86 ± 0.008 − 29 8573 orthogonal ML Magoulas et al. (2012)
g 1.08 ± 0.05 −0.74 ± 0.01 −8.033 ± 0.024 − 5825 direct ML Bernardi et al. (2003c)
r 1.17 ± 0.04 −0.75 ± 0.01 −8.022 ± 0.020 − 8228 direct ML Bernardi et al. (2003c)
i 1.21 ± 0.04 −0.77 ± 0.01 −8.164 ± 0.019 − 8022 direct ML Bernardi et al. (2003c)
z 1.20 ± 0.04 −0.76 ± 0.01 −7.995 ± 0.021 − 7914 direct ML Bernardi et al. (2003c)
g 1.12 ± 0.02 −0.74 ± 0.02 −8.046 − 46 410 direct R Hyde & Bernardi (2009)
r 1.17 ± 0.02 −0.76 ± 0.02 −8.086 − 46 410 direct R Hyde & Bernardi (2009)
i 1.20 ± 0.02 −0.76 ± 0.02 −8.048 − 46 410 direct R Hyde & Bernardi (2009)
z 1.23 ± 0.02 −0.78 ± 0.02 −8.216 − 46 410 direct R Hyde & Bernardi (2009)
I 1.25 ± 0.02 −0.79 ± 0.03 − 20 109 direct R Scodeggio et al. (1998)
R 1.13 ± 0.03 −0.84 ± 0.01 8.53 ± 0.1 − 699 direct R Fraix-Burnet et al. (2010)
u 0.798 ± 0.030 −0.700 ± 0.008 −7.53 ± 0.10 16.5 92 953 direct R this paper
g 0.966 ±  ± 0.030 −0.740 ± 0.013 −7.75 ± 0.13 15.6 92 953 direct R this paper
r 1.034 ± 0.030 −0.753 ± 0.013 −7.77 ± 0.13 15.3 92 953 direct R this paper
i 1.062 ± 0.030 −0.757 ± 0.013 −7.75 ± 0.13 15.0 92 953 direct R this paper
z 1.108 ± 0.030 −0.763 ± 0.013 −7.81 ± 0.13 14.8 92 953 direct R this paper

Notes. It is sorted by method (note: R = regression, ML = maximum likelihood) and date of publication. Some of the values in the list cannot be found in the same form due to slightly different definitions in the referenced papers. We sometimes had to renormalise the coefficient b, when the fundamental plane was defined using with the mean surface brightness μ0 instead of the parameter . Furthermore, the coefficient c, if available, is always given for a Hubble parameter of H0 = 70   km s-1 Mpc-1 here, therefore we had to rescale it if other values of H0 were used in the referenced paper. In addition to the fundamental plane coefficients a, b and if available c, the distance error σdist and the number of galaxies Ngal in the sample is given. Furthermore, we also list the type of fit (R = regression, ML = maximum likelihood), which was used to obtain the fundamental plane coefficient, because it is known that the coefficients not only depend on the wavelength, but also on the fitting method.

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