#Table 1 - Parameters of MC stellar "superclusters"
#
#SWB type  M_{K_s}(eff) M_{Ktip}   log age (yr)   log Z
#            [mag] +/-  [mag] +/-         +/-        +/-   
#
pre        -7.70 0.40   -8.7 0.2      6.4 0.3   -0.3 0.2
I          -8.85 0.12   -9.8 0.2      7.0 0.3   -0.3 0.2
II         -7.84 0.28   -8.9 0.2      7.5 0.3   -0.3 0.2
III        -7.45 0.24   -8.3 0.2      8.0 0.3   -0.1 0.2
IV         -7.51 0.18   -8.4 0.2      8.5 0.3   -0.8 0.2
V          -6.69 0.20   -8.0 0.2      9.0 0.3   -0.6 0.2
VI         -6.21 0.24   -7.6 0.2      9.5 0.3   -1.0 0.2
VII        -4.92 0.38   -7.2 0.2      9.9 0.3   -1.4 0.2
#
#Col.(2): M_{K_s}(eff) from Gonzalez et al. (2004, 2005).
#Col.(4): Ages from Frogel et al. (1990), corrected to the Large Magellanic 
#         Cloud distance modulus, (m-M)_o=18.5, as in Mouhcine et al.(2005); 
#         the age of the pre-SWB supercluster is also from Gonzalez et al.(2004). 
#Col.(5): Metallicities from Cohen (1982), for cluster types pre-SWB, 
#         I, and II, and from Frogel et al. (1990) for later types.