Evolution of the anti-truncated stellar profiles of S0 galaxies since $z=0.6$ in the SHARDS survey: I - Sample and Methods

@article{Borlaff2017EvolutionOT,
  title={Evolution of the anti-truncated stellar profiles of S0 galaxies since \$z=0.6\$ in the SHARDS survey: I - Sample and Methods},
  author={A. Borlaff and M. C. Eliche-Moral and J. Beckman and B. Ciambur and P. P'erez-Gonz'alez and G. Barro and A. Cava and N. Cardiel},
  journal={arXiv: Astrophysics of Galaxies},
  year={2017}
}
The controversy about the origin of the structure of S0--E/S0 galaxies may be due to the difficulty of comparing surface brightness profiles with different depths, photometric corrections and PSF effects (almost always ignored). We aim to quantify the properties of Type-III (anti-truncated) discs in a sample of S0 galaxies at 0.2<z<0.6. In this paper, we present the sample selection and describe in detail the methods to robustly trace the structure in their outskirts and correct for PSF effects… Expand
Evolution of the anti-truncated stellar profiles of S0 galaxies since $z=0.6$ in the SHARDS survey: II - Structural and photometric evolution.
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