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J/AJ/156/191
  The ages of M31 star clusters: SED versus CMD (Fan+, 2018)
img(gal)
    J/AJ/156/191/table1(c)Ages of our sample star clusters derived from SED fits of different passband combinations with BC03 models and Padova 2000 stellar evolutionary tracks (32 rows)
    J/AJ/156/191/table2Same as Table 1 but for fixed-Z from the literature (32 rows)
    J/AJ/156/191/table3Same as Table 1 but for the GALEV models and a Kroupa (2001MNRAS.322..231K) initial mass function (IMF) (32 rows)
    J/AJ/156/191/table4Same as Table 3 but for fixed-Z from the literature (32 rows)
    J/AJ/156/191/table5Same as Table 1 but for the ASPS bsp-SSPs models (32 rows)
    J/AJ/156/191/table6Same as Table 5 but for fixed-Z from the literature (32 rows)

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       (c)  indicates tables which contain celestial coordinates 
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