Spatial distribution of stellar mass and star formation activity at 0.2 < z < 1.2 across and along the main sequence

@article{Morselli2018SpatialDO,
  title={Spatial distribution of stellar mass and star formation activity at 0.2 < z < 1.2 across and along the main sequence},
  author={Laura Morselli and Paola Popesso and Anna Cibinel and Pascal A. Oesch and Mireia Montes and Hakim Atek and Garth D. Illingworth and Bradford P. Holden},
  journal={Astronomy \& Astrophysics},
  year={2018}
}
High-resolution multi-wavelength photometry is crucial to explore the spatial distribution of star formation in galaxies and understand how these evolve. To this aim, in this paper we exploit the deep, multi-wavelength Hubble Space Telescope (HST) data available in the central parts of the Great Observatories Origins Deep Survey (GOODS) fields and study the distribution of star formation activity and mass in galaxies located at different positions with respect to the main sequence (MS) of star… 

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