Table 4: Summary of the abundances derived in the programme stars. N, indicates the number of lines utilized for a specific element if more than one line was used (we then give the mean abundance together with its dispersion). [el/M] is the abundance ratio with respect to the mean derived [M/H] (see text and Table 3) and is only quoted for elements with $A\geq 30$.
    IGI95-C1     IGI95-C3     BMB-B 30  
Element N log $\epsilon$ $\rm {[el/M]}$ N log $\epsilon$ $\rm {[el/M]}$ N log $\epsilon$ $\rm {[el/M]}$
Li   <-0.50     -1.00     -0.80  
Ca   -     5.85     5.30  
Ti 3 $4.20\pm0.12$   2 $4.70\pm0.05$   4 $3.90\pm0.08$  
V 3 $3.10\pm0.15$   3 $3.50\pm0.15$     -  
Cr 2 $4.90\pm0.10$     5.32   2 $4.98\pm0.05$  
Mn   -     -   3 $4.39\pm0.05$  
Fe   6.85     -   3 $6.50\pm0.08$  
Ni 2 $5.50\pm0.10$   2 $5.85\pm0.05$     5.25  
Zn   4.00 0.20   4.10 0.00   4.00 0.40
Rb   <2.10 <0.50   -     1.40 0.00
Sr 2 $3.00\pm0.17$ 0.80 2 $3.35\pm0.05$ 0.90 2 $2.55\pm0.15$ 0.60
Y 2 $2.05\pm0.03$ 0.60   2.55 0.80 2 $1.65\pm0.02$ 0.40
Zr 4 $2.30\pm0.09$ 0.50 5 $3.30\pm0.20$ 1.20 4 $2.00\pm0.04$ 0.40
Nb   <0.72 <0.10   <1.20 <0.30   <0.42 <0.00
Ru 2 $1.50\pm0.10$ 0.50   -     1.45 <0.60
Ba   2.80 1.50   2.55a 0.80   2.60 1.50
La 5 $1.95\pm0.20$ 1.60   1.35 0.70 2 $1.50\pm0.15$ 1.40
Ce   <2.50 <1.70   -   2 $1.60\pm0.20$ 1.00
Pr 4 $1.10\pm0.04$ 1.20   -   2 $0.80\pm0.08$ 1.10
Nd 5 $2.50\pm0.12$ 1.80 2 $2.00\pm0.05$ 1.00 4 $2.10\pm0.11$ 1.60
Sm 2 $1.40\pm0.01$ 1.20 2 $1.50\pm0.10$ 0.90 2 $1.05\pm0.05$ 0.95
Gd   <1.50 <1.20   -     -  
Hf   1.00 0.90   -     1.10 1.20
W   1.20 0.90   -     0.50 0.40
a The Ba abundance derived in this star may be affected by the presence
  of Merrill-Sanford bands (see text).

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