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1 Introduction
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2 Observations and reductions
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3 ISOCAM results
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4 Near-IR and mid-IR excess YSOs
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5 Characterization of the YSO population
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6 Luminosity distribution
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7 Implications for the IMF in Serpens
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8 Spatial distributions
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9 Star formation rate and efficiency
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10 Summary and conclusions
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References
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Online Material
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Appendix A: Notes on some individual sources
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