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This article has an erratum: [https://doi.org/10.1051/0004-6361/201322953e]

Table 3

Temperatures and surface gravities for stars redder than the u-jump that do not show evidence of radiative levitation as derived from the a0 and sz parameters and from line profile fits for an assumed metallicity of [M/H] = −1.5.

ID Photometric parameters Spectroscopic parameters
a 0 sz T eff log g T eff log g
[mmag] [mmag] [K] [K]
52 +48 ± 4 91 ± 5 9100 ± 380 3.39 ± 0.11 8240 ± 20 2.87 ± 0.02
55 +124 ± 4 91 ± 4 8100 ± 260 3.08 ± 0.15
60 +134 ± 6 89 ± 7 8000 ± 260 3.05 ± 0.19
61 +151 ± 3 79 ± 3 7900 ± 210 3.09 ± 0.16
63 +125 ± 5 95 ± 5 8100 ± 270 3.02 ± 0.17
70 +82 ± 4 86 ± 4 8600 ± 330 3.36 ± 0.12 7990 ± 20 2.94 ± 0.03
72 +114 ± 7 86 ± 8 8200 ± 300 3.21 ± 0.18
74 +81 ± 3 85 ± 3 8600 ± 320 3.37 ± 0.11 7910 ± 10 2.94 ± 0.04
79 +79 ± 5 86 ± 5 8600 ± 340 3.37 ± 0.13 7990 ± 10 2.97 ± 0.03
81 +54 ± 3 84 ± 3 9000 ± 350 3.47 ± 0.10 8210 ± 20 2.98 ± 0.02
83 +34 ± 4 80 ± 4 9300 ± 400 3.57 ± 0.10 8360 ± 30 3.02 ± 0.02
86 +57 ± 3 84 ± 4 8900 ± 360 3.46 ± 0.10 8160 ± 20 3.00 ± 0.02
88 +30 ± 5 88 ± 6 9300 ± 420 3.46 ± 0.11 8390 ± 30 2.98 ± 0.02
89 +56 ± 3 81 ± 3 8900 ± 360 3.51 ± 0.10 8070 ± 20 2.93 ± 0.03
90 +27 ± 7 87 ± 10 9400 ± 470 3.48 ± 0.14 8450 ± 30 3.04 ± 0.02
96 +5 ± 7 84 ± 7 9700 ± 500 3.54 ± 0.12 8560 ± 30 3.07 ± 0.02
99 −17 ± 6 80 ± 7 10 100 ± 510 3.61 ± 0.12 9130 ± 260 3.25 ± 0.15 −0.6
102 0 ± 3 86 ± 3 9800 ± 440 3.51 ± 0.09 9290 ± 320 3.38 ± 0.18 −1.4
103 −56 ± 6 86 ± 7 10 900 ± 590 3.42 ± 0.19 9850 ± 70 3.34 ± 0.04 −1.0
106 −8 ± 5 84 ± 6 10 000 ± 490 3.54 ± 0.11 9230 ± 290 3.33 ± 0.17 −1.3
107 −5 ± 4 85 ± 4 9900 ± 460 3.52 ± 0.10 9350 ± 260 3.39 ± 0.15 −1.2
111 −52 ± 6 68 ± 6 10 800 ± 570 3.82 ± 0.12 9760 ± 90 3.44 ± 0.05 −1.0
113 −17 ± 3 85 ± 4 10 100 ± 470 3.52 ± 0.11 9210 ± 180 3.31 ± 0.11 −0.8
114 −27 ± 9 81 ± 11 10 300 ± 600 3.58 ± 0.17 9340 ± 140 3.33 ± 0.08 −1.0
115 −16 ± 4 86 ± 5 10 100 ± 480 3.50 ± 0.12 9280 ± 180 3.34 ± 0.10 −1.1
118 −27 ± 3 86 ± 3 10 300 ± 480 3.49 ± 0.11 9440 ± 90 3.38 ± 0.05 −1.1
119 −16 ± 3 87 ± 4 10 100 ± 470 3.48 ± 0.11 9430 ± 170 3.39 ± 0.09 −1.2
120 −32 ± 9 80 ± 10 10 400 ± 600 3.60 ± 0.17 9470 ± 70 3.39 ± 0.04 −1.0
122 −47 ± 7 77 ± 9 10 700 ± 590 3.64 ± 0.17 9740 ± 80 3.40 ± 0.04 −1.1
127 −63 ± 4 89 ± 4 11 000 ± 550 3.33 ± 0.18 9920 ± 80 3.37 ± 0.04 −0.8
143 −42 ± 5 84 ± 6 10 600 ± 550 3.50 ± 0.16 9810 ± 60 3.45 ± 0.03 −1.1
145 −46 ± 3 82 ± 3 10 700 ± 520 3.54 ± 0.12 9660 ± 60 3.42 ± 0.03 −1.0
147 −54 ± 4 73 ± 5 10 800 ± 550 3.71 ± 0.12 9810 ± 80 3.43 ± 0.04 −0.8
149 −67 ± 5 78 ± 5 11 100 ± 590 3.58 ± 0.17 9800 ± 80 3.41 ± 0.04 −1.0
151 −53 ± 4 72 ± 4 10 800 ± 540 3.74 ± 0.11 9760 ± 80 3.43 ± 0.04 −0.9
154 −51 ± 3 88 ± 4 10 800 ± 520 3.39 ± 0.15 10 100 ± 100 3.51 ± 0.04 −1.1
156 −46 ± 8 88 ± 10 10 700 ± 610 3.40 ± 0.22 9760 ± 80 3.37 ± 0.04 −1.0
157 −52 ± 11 79 ± 13 10 800 ± 670 3.59 ± 0.23 9580 ± 90 3.34 ± 0.05 −1.1
169 −88 ± 4 72 ± 5 11 600 ± 600 3.69 ± 0.17 10 400 ± 100 3.53 ± 0.05 −1.0
176 −72 ± 5 80 ± 6 11 200 ± 600 3.52 ± 0.19 10 300 ± 100 3.52 ± 0.05 −1.0
180 −75 ± 4 82 ± 5 11 300 ± 580 3.46 ± 0.18 10 600 ± 80 3.60 ± 0.04 −1.1

Notes. The errors for the photometric results are derived from the errors of a0 and sz in combination with the errors of the fits and an uncertainty of 002 for the reddening (see Sect. 5.1 for details). The errors for the spectroscopic results are derived from the χ2 fit (see Sect. 5.2 for details) and are only statistical errors. In addition, we list the helium abundance as determined with LINFOR (see Sect. 6 for details).

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