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Table 1:

Determination methods of radius, mass and age and background consideration.
Galaxy Radius determination Mass determination Background Age determination
LMC1 King profile fit from mass/light ratio from mean surface brightness combination of IMF 8
  half-surface brightness evolutionary code5 in annulus at $r \gg R_{\rm c}$ and evolutionary code5
SMC2 King profile fit from mass/light ratio from mean surface brightness Based on color-magnitude
  half-surface brightness evolutionary code5 in annulus at $r \gg R_{\rm c}$ diagram12
Antennae3 Fit with ISHAPE code6 UBVI-colors and mass/light Fit with ISHAPE code LICK line strength indices
    ratio7 with extinction-   and 11
    corrected SSP    
M 834 Fit with ISHAPE code6 Isochromes9 Fit with ISHAPE code UVBI-colors, 2-color and
        S-sequnce diagram 10

1 Mackey & Gilmore (2003a); 2 Mackey & Gilmore (2003b); 3 Mengel et al. (2008); 4 Larsen & Richter (2004); 5 Fioc & Rocca-Volmerangen (1997); 6 Larsen (1999); 7 Anders & Fritz-von-Alvensleben (2003); 8 Kroupa et al. (1993); 9 Girardi (2000); 10 Girardi (1995); 11 Schweizer (2005); 12 Chiosi (1995).


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