The Trace of the Assembly of Massive E-S0 Galaxies at 0.8<z<1.5 in Galaxy Number Counts
K-band galaxy number counts (GNCs) exhibit a slope change at K˜ 17.5 mag not present in optical bands. To unveil the nature of this feature we have derived the contribution of different galaxy types to the total K-band GNCs at 0.3 2) and evolved passively since then cannot predict the slope change, whereas models that impose a late definitive
Prieto, M. et al.
Fecha de publicación:
10
2016