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Table 2:

Coefficients of the FJR for the SDSS sample of galaxies in increasing-magnitude-intervals (lower magnitude cut-off).

MIa
Nb Bc Ad $\sigma_{\rm FJR}$e
Total SDSS sample (g filter)
$-23.5 \geq M > -24.5$ 325 1.082 $\pm$ 0.314 -23.132 $\pm$ 7.439 0.154
$-22.5 \geq M > -24.5$ 11 071 0.441 $\pm$ 0.014 -7.647 $\pm$ 0.311 0.267
$-21.5 \geq M > -24.5$ 48 432 0.242 $\pm$ 0.011 -2.999 $\pm$ 0.246 0.406
$-20.5 \geq M > -24.5$ 77 887 0.173 $\pm$ 0.009 -1.449 $\pm$ 0.208 0.532
$-19.5 \geq M > -24.5$ 87 949 0.152 $\pm$ 0.009 -0.976 $\pm$ 0.193 0.599
$-18.5 \geq M > -24.5$ 89 197 0.148 $\pm$ 0.009 -0.884 $\pm$ 0.195 0.615
$-17.5 \geq M > -24.5$ 89 308 0.147 $\pm$ 0.009 -0.867 $\pm$ 0.198 0.617
Total SDSS sample (r filter)
$-24.0 \geq M > -25.0$ 1081 0.525 $\pm$ 0.033 -10.232 $\pm$ 0.796 0.168
$-23.0 \geq M > -25.0$ 17 978 0.297 $\pm$ 0.015 -4.548 $\pm$ 0.2362 0.295
$-22.0 \geq M > -22.0$ 56 336 0.196 $\pm$ 0.011 -2.113 $\pm$ 0.248 0.431
$-21.0 \geq M > -25.0$ 81 344 0.157 $\pm$ 0.009 -1.208 $\pm$ 0.205 0.538
$-20.0 \geq M > -25.0$ 88 427 0.145 $\pm$ 0.008 -0.938 $\pm$ 0.192 0.585
$-19.0 \geq M > -25.0$ 89 245 0.143 $\pm$ 0.008 -0.876 $\pm$ 0.195 0.596
$-18.0 \geq M > -25.0$ 89 305 0.142 $\pm$ 0.008 -0.868 $\pm$ 0.197 0.598
Homogeneous SDSS sample (g filter)
$-22.5 \geq M > -23.0$ 14 1.038 $\pm$ 0.206 -20.988 $\pm$ 4.675 0.056
$-21.5 \geq M > -23.0$ 1823 0.505 $\pm$ 0.022 -8.666 $\pm$ 0.487 0.218
$-20.5 \geq M > -23.0$ 9386 0.287 $\pm$ 0.019 -3.796 $\pm$ 0.397 0.371
$-19.5 \geq M > -23.0$ 16 162 0.211 $\pm$ 0.016 -2.138 $\pm$ 0.339 0.498
$-18.5 \geq M > -23.0$ 16 901 0.196 $\pm$ 0.017 -1.849 $\pm$ 0.349 0.531
Homogeneous SDSS sample (r filter)
$-23.0 \geq M > -23.5$ 82 0.629 $\pm$ 0.071 -12.142 $\pm$ 1.647 0.109
$-22.0 \geq M > -23.5$ 3005 0.376 $\pm$ 0.026 -6.084 $\pm$ 0.571 0.255
$-21.0 \geq M > -23.5$ 11 293 0.242 $\pm$ 0.019 -2.989 $\pm$ 0.404 0.398
$-20.0 \geq M > -23.5$ 16 514 0.197 $\pm$ 0.016 -2.003 $\pm$ 0.346 0.498
$-19.0 \geq M > -23.5$ 16 910 0.189 $\pm$ 0.016 -1.829 $\pm$ 0.354 0.519

Notes. (a) Absolute magnitude interval within which the galaxies are distributed. (b) Number of galaxies in the magnitude interval. (c) Slope of the FJR. (d) Zero point of the FJR. (e) Total intrinsic dispersion of the FJR.


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