Sample | Filter | N |
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(1) | (2) | (3) | (4) | (5) | (6) | (7) |
BL (this work) | H | 23 | 0.155 ![]() |
-24.5 ![]() |
-25.8 ![]() |
7.8 ![]() |
BL C03 | K | 8 | 0.186 ![]() |
-25.6 ![]() |
-26.0 ![]() |
4.2 ![]() |
BL S00 | H | 9 | 0.206 ![]() |
-25.0 ![]() |
-26.2 ![]() |
10 ![]() |
BL K98 | H | 7 | 0.112 ![]() |
-25.7 ![]() |
-25.8 ![]() |
4.8 ![]() |
BL all | H/K | 42 | 0.164 ![]() |
-25.0 ![]() |
-25.9 ![]() |
7.2 ![]() |
L* Mobasher et al. (1993) | K | 136 | 0.077 ![]() |
-25.0 ![]() |
||
BCM Thuan & Puschell (1989) | H | 84 | 0.074 ![]() |
-26.3 ![]() |
||
BCM Aragon-Salamanca et al. (1998) | K | 25 | 0.449 ![]() |
-27.0 ![]() |
||
RG FR II Taylor et al. (1996) | K | 12 | 0.214 ![]() |
-25.1 ![]() |
-26.1 ![]() |
26 ![]() |
RG Willott et al. (2003) z < 0.3 | K | 42 | 0.170 ![]() |
-26.2 ![]() |
a Column (1) gives the sample; Col. 2: the filter; Col. 3: the number of objects in the sample; Col. 4: the average redshift of the sample; Cols. 5 and 6: the average H band nuclear and host galaxy absolute magnitude of the sample; and Col. 7: the average H-band bulge scale length of the sample. |