Barro, GuillermoGallego Maestro, JesúsPérez González, Pablo GuillermoEliche Moral, María del CarmenBalcells, M.Villar, V.Cardiel López, NicolásCristobal Hornillos, D.Gil de Paz, ArmandoGuzmán, R.Pelló, R.Prieto, M.Zamorano Calvo, Jaime2023-06-202023-06-2020101570-659110.1007/978-3-642-11250-8_29https://hdl.handle.net/20.500.14352/43001© Springer-Verlag Berlin Heidelberg 2010. Scientific Meeting of the Spanish-Astronomical-Society (SEA) (8th; 2008; Santander-SPAIN)We present a study that links the NCs to the rest-frame luminosity functions (LFs) at the passbands probed by the observed K-band at different epochs. Making use of a large K-band selected sample in the Groth Field, HDFN and CDFS (∼0.27deg^(2)), we have derived highly reliable photometric redshift estimates that allow us to estimate LFs in the redshift range [0.25-1.25]. We find that the larger flattening in the slope of the K-band NCs is mostly a consequence of a prominent decrease in the characteristic density (φ∗) around z∼1, and an almost flat evolution of M∗.engjournal articlehttp://dx.doi.org/10.1007/978-3-642-11250-8_29https://link.springer.com/restricted access52AstronomyAstrophysicsAstrofísica