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Table 1:

Identification of programme stars and the derived elemental abundances.

ID
RA Dec V [Fe/H] [Fe/H] $\epsilon$(Fe) $\epsilon$(Mg)   $\epsilon$(Ca) $\epsilon$(Ba)
  (J2000.0) (J2000.0)   (7.45) Norris08          
Boo-007 13 59 35 +14 20 23 17.88 -2.28 -2.32 5.17  0.26 (22) 5.68  0.18 (4) 5.57 4.24  0.22 (5) -0.90 (1)
Boo-033 14 00 11 +14 25 01 17.79 -2.47 -2.96 4.98  0.36 (25) 5.53  0.30 (4) 5.77 4.22  0.28 (5) -0.74  0.24 (2)
Boo-094 14 00 31 +14 34 03 16.99 -2.90 -2.79 4.55  0.22 (25) 5.14  0.04 (4) 5.12 3.61  0.03 (4)  
Boo-117 14 00 10 +14 31 45 17.74 -2.24 -1.72 5.21  0.30 (21) 5.66  0.23 (3) 5.53 4.34  0.28 (4) -0.57  0.11 (2)
Boo-121 14 00 36 +14 39 27 17.42 -2.39 -2.37 5.06  0.22 (26) 5.53  0.30 (4) 5.78 4.28  0.29 (5) -0.69 (1)
Boo-127 14 00 14 +14 35 52 17.69 -1.98 -1.49 5.47  0.34 (29) 6.28  0.11 (3) 6.33 4.33  0.18 (5) -0.49  0.43 (2)
Boo-911 14 00 01 +14 36 51 17.49 -2.21 -1.98 5.24  0.29 (29) 5.63  0.24 (4) 5.45 4.48  0.05 (4) -0.64  0.09 (2)


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