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Table 1.

Parameters of the Sérsic law fits on the surface brightness profiles for both cEs.

Name μeff, B reff, B nB B0 μeff, I reff, I nI I0
(magarcsec−2) (arcsec) (mag) (magarcsec−2) (arcsec) (mag)
Single component

FS90 110 20.29 ± 0.07 1.25 ± 0.04 3.00 ± 0.12 16.57 18.06 ± 0.06 1.20 ± 0.03 2.81 ± 0.08 14.45
FS90 192 22.06 ± 0.06 1.62 ± 0.03 2.21 ± 0.08 17.93 19.79 ± 0.05 1.51 ± 0.03 2.22 ± 0.07 15.81

Three components

FS90 110
Nuclear 18.09 ± 0.06 0.26 ± 0.01 1.45 ± 0.08 18.28 16.09 ± 0.07 0.29 ± 0.01 1.37 ± 0.06 15.93
Inner 20.38 ± 0.04 1.29 ± 0.02 0.87 ± 0.04 17.20 18.28 ± 0.06 1.30 ± 0.03 0.81 ± 0.04 15.11
Outer 23.94 ± 0.12 4.65 ± 0.14 0.48 ± 0.06 18.20 21.85 ± 0.07 4.52 ± 0.10 0.55 ± 0.04 16.14
FS90 192
Nuclear 21.34 ± 0.13 0.27 ± 0.03 1.79 ± 0.17 21.21 18.95 ± 0.15 0.29 ± 0.02 1.89 ± 0.22 18.66
Inner 23.69 ± 0.10 1.63 ± 0.05 0.31 ± 0.04 20.36 21.29 ± 0.11 1.55 ± 0.06 0.44 ± 0.06 17.97
Outer 21.47 ± 0.20 1.84 ± 0.44 2.01 ± 0.20 18.11 20.35 ± 0.18 1.80 ± 0.35 1.96 ± 0.24 16.05

Notes. The table includes the effective surface brightness for the galaxies (μeff), the effective radius (reff), the Sérsic index (n), and the integrated magnitude in the B and I filters, corrected for extinction following Schlafly & Finkbeiner (2011). For each galaxy, both the case of a single Sérsic law and the fit assuming three components are considered.

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