... 6872

Based on Observations at the Very Large Telescope of the European Southern Observatory, Paranal/Chile under Program 71.B-0596.

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...

Complete Table 2, containing the photometry, positions, and derived properties of each source is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/435/65

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...2003b

Note that the exponents of mass functions and luminosity functions have been combined here. If the cluster population is close to a single aged population then $\alpha$ is the same for the mass and luminosity functions. For a detailed analysis of the luminosity function of young cluster systems see Gieles et al. (2005).

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... to 100

The mass of the Pavo group was estimated using its measured temperature of 0.82 keV (Davis et al. 1999), which is typical of poor galaxy clusters with masses of a few times $10^{13}~M_{\odot}$ (Mulchaey et al. 1996).

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