It is shown that the class of asymptotically flat solutions to the axisymmetric and stationary vacuum Einstein equations with reflection symmetry of the metric is uniquely characterized by a simple relation for the Ernst potential on the upper part of the symmetry axis ( axis): . This result generalizes a well-known fact from potential theory: axisymmetric solutions to the Laplace equation that vanish at infinity and have reflection symmetry with respect to the plane are characterized by a potential that is an odd function of on the upper part of the axis.
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