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1 Introduction
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2 The FORS deep field
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3 I selection versus K selection
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4 Photometric redshifts
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5 Luminosity functions
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6 Parameterizing the evolution of the luminosity function
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7 Comparison with the literature
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8 Comparison with model predictions
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9 Summary and conclusions
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Appendix B: Comparison with literature
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References
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Online Material
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Appendix A: Schechter parameters
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Appendix C: Confidence levels for the slope
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