Back to the Abstract

	1 Introduction
	2 The K20 spectroscopic sample
	3 The estimate of the rest-frame near-IR luminosities
	4 The estimate of the near-IR Luminosity Function
	5 The cosmic evolution of the near-IR Luminosity Function
	6 The Luminosity Function by spectral or color type
	7 The near-IR luminosity density evolution
	8 The comparison with model predictions
	9 Summary and discussion
	References

	List of tables
	List of figures