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1 Introduction
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2 Experimental setup, observations and data reduction
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3 The bright-star sample
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4 Candidate selection from the bright-star sample
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5 Candidate sample and verifications
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6 The status of published Magellanic microlensing candidates
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7 The detection efficiency
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8 Limits on the abundance of machos
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9 Discussion of the results
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References
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Online Material
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Appendix A: Candidate selection for the full sample
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