Strong size evolution of the most massive
galaxies since z~2
Nine billions years ago massive
spheroid-like objects were much smaller than those we see today. These
small sized, high mass galaxies do not exist in the nearby universe,
suggesting this population merged with other galaxies over several
billion years to form the largest galaxies we see today.

Size evolution of equal stellar
mass objects at different lookback times (from top-right to
bottom-left: 3.9, 5.3, 7.4, 9.0, 9.7 and 10.3 Gyr back
respectively). Effective radii are given in kpc and stellar masses in
10¹¹ solar masses units. Galaxies are shown with different
surface brightness limits to account for the cosmological surface
brightness dimming. The solid line indicates one arcsec angular size.