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Table 1.

Coefficients and associated uncertainties of the polynomial fits to the size–magnitude relations for the various components of the single profile fits or bulge and disk decompositions for different EFIGI morphological subsamples, and dispersion in the residuals from these fits.

Type Component Band Size–magnitude relation Dispersion in residual
Polynomial fit (a)
Polynomial fit (b)
2nd order 1st order 0th order 2nd order 1st order 0th order
cD Single-Sérsic g −0.28±0.05 −1.79±1.03 0.18±0.03
i −0.28±0.04 −2.06±0.93 0.18±0.03
dE Single-Sérsic g −0.20±0.03 −0.32±0.49 0.24±0.03
i −0.19±0.03 −0.15±0.48 0.23±0.03
E Single-Sérsic g −0.37±0.04 −3.95±0.37 0.24±0.02(c)
0.062±0.010 2.27±0.42 24.09±4.46 0.21±0.02
i −0.32±0.02 −3.16±0.46 0.23±0.02
0.053±0.012 2.04±0.53 23.02±5.85 0.22±0.02
E Sérsic g −0.28±0.01 −2.46±0.24 0.15±0.01
i −0.24±0.02 −1.91±0.34 0.14±0.01
E to Sm Sérsic or bulge g 0.025±0.001 0.76±0.05 8.25±0.50 0.027±0.003(d) 0.76±0.06(d)
i 0.026±0.001 0.83±0.05 9.35±0.52 0.039±0.002(d) 1.03±0.05(d)
E and cD Exponential g −0.249±0.012 −1.12±0.27 0.18±0.01
i −0.243±0.011 −1.26±0.26 0.18±0.01
S0 to Scd Disk g −0.208±0.004 −0.43±0.08 0.175±0.004
i −0.214±0.004 −0.73±0.09 0.170±0.004
Sd to Im Disk g −0.140±0.007 0.98±0.14 0.019±0.009 0.59±0.16
i −0.151±0.007 0.71±0.15 0.018±0.010 0.58±0.18
E to Im Exponential, disk or single-Sérsic g 0.020±0.002 0.63±0.08 8.29±0.81 0.0043±0.0013(d) 0.18±0.05(d) 2.17±0.45(d)
i 0.032±0.002 1.17±0.09 14.34±0.91 0.013±0.001(d) 0.55±0.06(d) 6.04±0.57(d)

Notes.

(a)

Coefficients of the polynomials obtained by ODR fitting of the profile effective radius (in log) versus magnitude, for a sample of EFIGI galaxies defined by their morphological types, in the listed band. Bulge (or Sérsic) and disk (or exponential) refer to the corresponding component in the bulge and disk decomposition. When indicated, E, cD, dE and Im galaxies are modeled as single Sérsic profiles (see Sect. 3.1).

(b)

Coefficients of the polynomials providing the rms dispersion (in dex) around the size–magnitude relation fit.

(c)

The center and χ2 of the Gaussian fit to the residuals of the elliptical size–luminosity relation appear in the descriptive text in Sect. 4.2.

(d)

The Gaussian fits to the residuals of the bulge and disk 2nd degree polynomial size–luminosity relations are shown in the right panels of Figs. 8 and 12, respectively, and their centers and χ2 values appear in the descriptive texts in Sects. 4.3 and 4.5, respectively.

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