Color Gradients in Galaxies Out to z~3: Dependence on Galaxy Properties
  Using HST/ACS observations, we measure the color gradients of 3248 galaxies in the GOODS-South field out to z~3 and i_{AB}<25.5 and characterize their dependence on galaxy properties (luminosity, apparent magnitude, galaxy size, redshift and morphological type). The color gradient is measured by the difference of v-i color outside (R_{50}<r<2R_{50}) and inside the half light radius. The gradient shows little evolution with redshift up to z~1 but increases from z~1 to z~2 before flattening out. It also increases with apparent magnitude, with a median value of 0.24 magnitudes at i_{AB}~25.5. It has a strong color dependence, with the bluest galaxies (in terms of observed color) having cores that are bluer relative to their outskirts. We probe the redshift evolution by stacking galaxies and measuring the radial variation of v-i color within them. At low redshifts (z<0.5), the centres of galaxies (r<R_{50}) are slightly redder than their outskirts (1.5R_{50}<r<2R_{50}). Galaxies at z~1 and -22.0<M_I<-21.0 are bluer in their cores by 0.1 magnitudes, on average, compared to their outskirts. For z>1, galaxies show increasingly bluer cores while the color of the outskirts does not change as rapidly. At z~2.5 and -22.0<M_I<-21.0, we observe a difference, on average, of 0.4 magnitudes between the centre and the outskirts. The observed color gradients may indicate that strong star formation in galaxies at z>=2 is concentrated in their central regions. These color gradients and their dependence on galaxy properties could also have a significant impact on shear measurements in upcoming weak lensing cosmological surveys. 
Niraj Welikala (IAS, Orsay), Jean-Paul Kneib (LAM)
astro-ph.CO