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J/A+A/642/A176
  Chemical evolution of dSph galaxy Sextans (Theler+, 2020)
img(gal)
    J/A+A/642/A176/table2(c)Position, photometry and radial velocities of our targets (112 rows)
    J/A+A/642/A176/table3Parameters derived from photometry for the probable members of our sample (89 rows)
    J/A+A/642/A176/table4The radial velocities measured by DAOSPEC in each of the HR10, HR13, HR14 setups, and their average (110 rows)
    J/A+A/642/A176/table5Equivalent widths of the stars observed with UVES (205 rows)
    J/A+A/642/A176/table6Four stellar parameters for the probables members of our sample (89 rows)
    J/A+A/642/A176/table9Complete line list used to derive all the atomic abundances (268 rows)
    J/A+A/642/A176/table10*Atomic abundances for Fe, Mg, Ca and Sc (Note) (87 rows)
    J/A+A/642/A176/table11*Atomic abundances for TiI, TiII, Cr and Mn (Note) (87 rows)
    J/A+A/642/A176/table12*Atomic abundances for TiI, TiII, Cr and Mn (Note) (87 rows)
    J/A+A/642/A176/table13Equivalent widths of the GIRAFFE sample (34 rows)

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       (c)  indicates tables which contain celestial coordinates 
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