The K20 survey. V. The evolution of the near-IR Luminosity Function

The K20 survey. V. The evolution of the near-IR Luminosity Function

We present the galaxy rest-frame near-IR Luminosity Function (LF) and its cosmic evolution to $z\sim1.5$ based on a spectroscopic survey of a magnitude limited sample of galaxies with $K_{\rm s}

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2003-05, Vol.402 (3), p.837-848
Hauptverfasser: Pozzetti, L., Cimatti, A., Zamorani, G., Daddi, E., Menci, N., Fontana, A., Renzini, A., Mignoli, M., Poli, F., Saracco, P., Broadhurst, T., Cristiani, S., D'Odorico, S., Giallongo, E., Gilmozzi, R.
Format: Artikel
Sprache:eng
Schlagworte:
cosmology: observations
evolution
formation
galaxies: elliptical and lenticular
infrared: galaxies
luminosity function
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Beschreibung
Zusammenfassung:We present the galaxy rest-frame near-IR Luminosity Function (LF) and its cosmic evolution to $z\sim1.5$ based on a spectroscopic survey of a magnitude limited sample of galaxies with $K_{\rm s}
ISSN:0004-6361
1432-0746
DOI:10.1051/0004-6361:20030292