We study the extreme Lp\documentclass[12pt]{minimal}
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\begin{document}$$L_p$$\end{document} discrepancy of infinite sequences in the d-dimensional unit cube, which uses arbitrary sub-intervals of the unit cube as test sets. This is in contrast to the classical star Lp\documentclass[12pt]{minimal}
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\begin{document}$$L_p$$\end{document} discrepancy, which uses exclusively intervals that are anchored in the origin as test sets. We show that for any dimension d and any p>1\documentclass[12pt]{minimal}
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\begin{document}$$p>1$$\end{document}, the extreme Lp\documentclass[12pt]{minimal}
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\begin{document}$$L_p$$\end{document} discrepancy of every infinite sequence in [0,1)d\documentclass[12pt]{minimal}
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\begin{document}$$[0,1)^d$$\end{document} is at least of order of magnitude (logN)d/2\documentclass[12pt]{minimal}
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\begin{document}$$(\log N)^{d/2}$$\end{document}, where N is the number of considered initial terms of the sequence. For p∈(1,∞)\documentclass[12pt]{minimal}
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\begin{document}$$p \in (1,\infty )$$\end{document}, this order of magnitude is best possible.