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1 Introduction
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2 Selection of the AGN and X-ray binary sample
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3 Determination of the basic source parameters
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4 Source classification and parameter determination in the
hardness ratio plane
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5 Constraining intervening LMC gas columns
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6 The X-ray binary sample
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7 Summary and conclusions
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Appendix A: X-ray sources in a deep merged observation of the northern field
of the supergiant shell LMC 4
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References
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