Table 2: Journal of spectropolarimetric observations of HD 24712. The longitudinal field $\langle B_{\rm z} \rangle$ was estimated using ten Nd II and Nd III lines (3rd column), and seven Cr I, Cr II, and Fe I lines (4th column).
HJD Rotation $\langle B_{\rm z} \rangle$ (G)
(2 450 000+) phase Nd II, Nd III Cr I, Cr II, Fe I
2 941.6516 0.44 $ 598\pm 165$ $ 87\pm ~~68$
2 943.6341 0.60 $ 909\pm 154$ $ 240\pm 132$
2 945.5758 0.76 $1109\pm 105$ $ 535\pm 145$
2 946.5973 0.84 $1090\pm 144$ $ 729\pm 180$
2 947.6067 0.92 $1182\pm 100$ $1098\pm ~~98$
2 948.6514 0.00 $1132\pm ~~98$ $1064\pm 130$
2 952.6267 0.32 $ 835\pm 174$ $ 258\pm ~~79$
2 953.6572 0.40 $ 629\pm 129$ $ 155\pm ~~86$
2 954.6316 0.48 $ 720\pm 192$ $ 165\pm 155$
2 955.6350 0.56 $ 830\pm 187$ $ 137\pm 107$
2 956.5954 0.64 $1062\pm 178$ $ 260\pm 174$
2 957.5958 0.72 $1159\pm 164$ $ 483\pm 158$
2 961.6160 0.04 $1168\pm 100$ $1048\pm 152$


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