List of the specific frequencies SN,UCD derived in Sect. 3, along with the total absolute magnitude of the host environments.
|Centaurus||5.1 ± 1.7||–23.2||–23.2||0.38||7.3 ± 1.5*|
|Fornax||4.9 ± 1.7||–23.0||–22.6||0.54||5.1 ± 1.2**|
|Hydra||12.5 ± 4.3||–22.9||–22.5||0.58||12.5 ± 1.5***|
|HCG 90||1.3 ± 0.7||–22.4||–21.1||1.41|
|HCG 22||3.9 ± 1.6||–21.6||–21.1||1.41|
|Local Group||4.1 ± 1.5||–21.5||–21.0||1.5||1.8 ± 0.3****|
Notes. MV,host includes the full galaxy light in the UCD survey area (see text). MV,host,individual gives the magnitude of the brightest galaxy in the environment, which defines the assumed width σ of the GCLF and hence the correction term cw. The last column gives the literature value for the GC specific frequency of the brightest cluster galaxy, where available.
Mieske et al. (2005);
Dirsch et al. (2003);
Wehner et al. (2008);
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