The bright end of the z  ~ 7 UV luminosity function from a wide and deep HAWK-I survey

Aims. We perform a deep search for galaxies in the redshift range 6.5 ≤ z ≤ 7.5 to measure the evolution of the number density of luminous galaxies in this redshift range and derive useful constraints on the evolution of their luminosity function. Methods. We present here the second half of an ESO L...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2010-12, Vol.524, p.A28
Hauptverfasser:	Castellano, M., Fontana, A., Paris, D., Grazian, A., Pentericci, L., Boutsia, K., Santini, P., Testa, V., Dickinson, M., Giavalisco, M., Bouwens, R., Cuby, J.-G., Mannucci, F., Clément, B., Cristiani, S., Fiore, F., Gallozzi, S., Giallongo, E., Maiolino, R., Menci, N., Moorwood, A., Nonino, M., Renzini, A., Rosati, P., Salimbeni, S., Vanzella, E.
Format:	Artikel
Sprache:	eng
Schlagworte:	galaxies: distances and redshifts galaxies: evolution galaxies: high-redshift galaxies: luminosity function mass function
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