Statistics for Kinematic analysis of a sample of X-ray luminous distant galaxy clusters The L<sub>x</sub>-σ<sub>v</sub> relation in the <i>z</i> &gt; 0.6 universe

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Kinematic analysis of a sample of X-ray luminous distant galaxy clusters The L<sub>x</sub>-σ<sub>v</sub> relation in the <i>z</i> &gt; 0.6 universe 0

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