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Table 7

Bulge magnitudes and black hole masses.

Name Abs. magnitude log   (MBH,Hβ/M) M/Lλ ratio Fraction of


M J,bul M H,bul M K,bul J H K 0.1 Gyr population

08 HE0045-2145 −20.36 −21.88 −22.42 5.89 0.22 0.07 0.05 >70%
11 HE0103-5842 −22.50 −23.37 −23.78 6.71 0.16 0.10 0.07 >70%
24 HE0224-2834 −23.43 −24.15 −24.48 7.63 0.46 0.32 0.24 40−80%
29 HE0253-1641 −20.78 −21.80 −22.13 6.71 0.80 0.42 0.32 10−30%
71 HE1310-1051 −22.12 −22.86 −23.25 7.33 0.84 0.57 0.41 10−30%
75 HE1338-1423 −23.44 −23.88 −23.97 7.30 0.23 0.21 0.20 >70%
77 HE1348-1758 −21.09 −21.77 −21.99 6.30 0.26 0.19 0.16 >70%
79 HE1417-0909 −21.97 −22.74 −23.05 7.24 0.80 0.52 0.41 10−30%
81 HE2128-0221 −22.49 −22.97 −23.36 7.40 0.69 0.59 0.43 10−30%
82 HE2129-3356 −22.10 −22.68 −23.23 7.80 2.23 1.75 1.10 0%
83 HE2204-3249 −24.01 −24.68 −25.00 8.11 0.72 0.52 0.40 10−30%

Notes. Measured J-, H-, and K-band magnitudes of the spheroidal component (Cols. 2−4) and the BH masses (Col. 5). Columns 6−8 show M/Lλ ratios, which are necessary to shift galaxies on the MBH − Mbulge relation of inactive galaxies. Column 9 shows an estimate of the mass fraction of the 0.1 Gyr population that has to be added to an old 10 Gyr population to reproduce the observed M/Lλ ratios.

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