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J/A+A/660/A88
  Abundances of Local Group globular clusters (Larsen+, 2022)
img(gal)
    J/A+A/660/A88/sources(c)List of studied clusters + Arcturus and the Sun (with data in tablef1.dat) (47 rows)
    J/A+A/660/A88/tableb1Spectral window definitions (129 rows)
    J/A+A/660/A88/tablec1Mean DSEP NLTE abundances: Fe, Na, Mg, Si, Ca, Ti (45 rows)
    J/A+A/660/A88/tablec2Mean DSEP NLTE abundances: Sc, Cr, Mn, Ni (45 rows)
    J/A+A/660/A88/tablec3Mean DSEP NLTE abundances: Cu, Zn, Zr, Ba, Eu (45 rows)
    J/A+A/660/A88/tabled1Mean DSEP LTE abundances: Fe, Na, Mg, Si, Ca, Ti (45 rows)
    J/A+A/660/A88/tabled2Mean DSEP LTE abundances: Sc, Cr, Mn, Ni (45 rows)
    J/A+A/660/A88/tabled3Mean DSEP LTE abundances: Cu, Zn, Zr, Ba, Eu (45 rows)
    J/A+A/660/A88/tablee1Mean BaSTI NLTE abundances: Fe, Na, Mg, Si, Ca, Ti (45 rows)
    J/A+A/660/A88/tablee3Mean BaSTI NLTE abundances: Cu, Zn, Zr, Ba, Eu (45 rows)
    J/A+A/660/A88/tablee2Mean BaSTI NLTE abundances: Sc, Cr, Mn, Ni (45 rows)
    J/A+A/660/A88/tablef1Individual abundance measurements (DSEP) (5685 rows)

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       (c)  indicates tables which contain celestial coordinates 
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