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Table A.8

Median abundance, standard deviation, total error and number of lines used for NGC 6802 giant cluster members.

Median σa δtot Nlines b

[Fe i/H] 0.07 0.02 169
[Fe ii/H] 0.07 0.05 28
[C/Fe] 0.16 0.05 0.10 2
[N/Fe] 0.51 0.05 0.13 3
[O/Fe] 0.01 0.08 0.11 1
[Na/Fe] 0.49 0.09 0.12 5
[Mg/Fe] 0.09 0.04 0.17 5
[Al/Fe] 0.18 0.03 0.13 3
[Si/Fe] 0.04 0.03 0.12 8
[S/Fe] 0.01 0.05 0.12 1
[Ca/Fe] 0.02 0.03 0.13 26
[Sc/Fe] 0.01 0.06 0.17 6
[Ti/Fe] 0.04 0.04 0.13 65
[V/Fe] 0.06 0.03 0.13 30
[Cr/Fe] 0.04 0.03 0.18 37
[Mn/Fe] 0.01 0.07 0.17 14
[Co/Fe] 0.04 0.02 0.16 25
[Ni/Fe] 0.04 0.02 0.15 41
[Zn/Fe] 0.22 0.13 0.16 2
[Y/Fe] 0.03 0.06 0.14 13
[Zr/Fe] 0.08 0.12 0.17 6
[Mo/Fe] 0.05 0.21 0.14 2
[Ba/Fe] 0.13 0.05 0.18 3
[La/Fe] 0.06 0.09 0.18 4
[Ce/Fe] 0.00 0.08 0.19 4
[Nd/Fe] 0.16 0.08 0.19 10
[Eu/Fe] 0.07 0.07 0.19 1

Notes.

(a)

Standard deviations;

(b)

median numbers of spectral lines used. Note that the available spectral lines in UVES spectra are greater or equal to these numbers.

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