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1 Introduction
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2 Observations and data reduction
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3 The completeness and detection limit of the ADONIS and NACO surveys
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4 Status of the stellar components
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5 Masses and mass ratios
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6 The lower end of the companion mass distribution
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7 Binarity and multiplicity in Sco OB2
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8 Conclusions
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References
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Online Material
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Appendix A: Results of the NAOS/CONICA survey
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