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Table 2

Logbook of the observations and the results of the magnetic field measurements for all targets in our sample.

HD Spectral mV MJD S/N Line FAP Det. Bz Remark
number type mask flag [G]
61954 B9* 9.44 60311.14 127 Si 7.4 × 10−5 MD −420 ± 95 BSS, NGC2437
60315.06 98 HeCSi 2.8 × 10−6 DD 156 ± 46
62000 A1II/III 9.23 60311.27 156 Fe <10−10 DD −4± 29 YSS, NGC2437
Ti 1.4 × 10−5 MD −111 ± 43
62329 A2* 9.24 60312.24 121 Fe 9.3 × 10−5 MD 114± 87 YSS, NGC2437
60314.09 96 Fe 1.5 × 10−6 DD −582± 86
62775 A2III/IV 8.12 60312.06 133 Fe 6.4 × 10−5 MD 631 ± 110 BSS, NGC2447
60314.12 182 FeTi 1.1 × 10−7 DD
65032 A2/3III 8.35 60312.11 126 Fe 0.5 × 10−5 MD Likely YSS, Trumpler9
60313.09 132 SiCr 7.8 × 10−8 DD
87222 B3IV 8.63 60313.16 137 HeC 8.1 × 10−4 MD −133±7 BSS, NGC3114
87266 B3III/V 8.23 60315.19 164 CNNeSi 1.0 × 10−5 DD 110 ± 23 BSS, NGC3114
101545A O9.5Ib 6.38 60311.32 194 HeNOSi 2.1 × 10−5 MD 69 ± 17 BSS, IC2944
He 4.3 × 10−6 DD 82 ± 16

Notes. The first column gives the HD number of the star followed by the spectral type taken either from SIMBAD or from Cannon & Pickering (1993) (marked by *) and the visual magnitude. The fourth column presents the MJD values at the middle of the exposure, while in the fifth column we show the signal-to-noise ratio measured in the Stokes I spectra in the spectral region around 5000 Å. The applied line masks, the FAP values, the detection flag – where DD means definite detection, MD marginal detection, and ND no detection – the measured LSD mean longitudinal magnetic field strength, and a remark on cluster membership are presented in columns 6–10.

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