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J/A+A/669/A119
  Radial abundance gradient with open clusters (Magrini+, 2023)
  
    J/A+A/669/A119/tablea1SlopesIDR6 solar and M67 abundances (24 rows)
    J/A+A/669/A119/tablea2Average [alphaH] and [alpha/Fe] for our sample of open clusters (62 rows)
    J/A+A/669/A119/tablea3Average [odd/H] and [odd/Fe] for our sample of open clusters (62 rows)
    J/A+A/669/A119/tablea4Average [iron peak/H] and [iron peak/Fe] for our sample of open clusters. (62 rows)
    J/A+A/669/A119/tablea5Average [s/H] and [s/Fe] for our sample of open clusters (62 rows)
    J/A+A/669/A119/tablea6Average [r/H] and [r/Fe] for our sample of open clusters (62 rows)
    J/A+A/669/A119/tablea7Number of member stars in each cluster and for each element used in this work (62 rows)
    J/A+A/669/A119/tablea8Linear weighed regression fitting coefficients of [El/H]=m1.RGC+c for the open clusters in the two investigated galactocentric regions and in the whole distance range (25 rows)
    J/A+A/669/A119/tablea9Linear weighed regression fitting coefficients of [El/Fe]=m1.RGC+c for the open clusters in the two investigated galactocentric regions and in the whole distance range (24 rows)
    J/A+A/669/A119/tablea10Linear weighed regression fitting coefficients of [El/H]=m1.RGC+c for the open clusters in the three investigated age bins (25 rows)
    J/A+A/669/A119/tablea11Linear weighed regression fitting coefficients of [El/Fe]=m1.RGC+c for the open clusters in the three investigated age bins. (24 rows)

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