International audienceHigh-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-forming galaxies. Our sample consists of galaxies with stellar mass ≥109.5 M⊙ in the redshift range 0.2 ≤ z ≤ 1.2. Exploiting 10-band photometry from the UV to the near-infrared at HST resolution, we derived spatially resolved ma...
For a mass-selected sample of 66544 galaxies with photometric redshifts (z phot) from the Cosmic Evo...
The assembly of galaxies can be described by the distribution of their star formation as a function ...
We present an analysis of the spatial distribution of star formation in a sample of 60 visually iden...
International audienceHigh-resolution multi-wavelength photometry is crucial to explore the spatial ...
High-resolution multi-wavelength photometry is crucial to explore the spatial distribution of star f...
Using spatially resolved Hα emission line maps of star-forming galaxies, we study the spatial distri...
We perform the first spatially-resolved stellar population study of galaxies in the early universe z...
We investigate the relation between the star formation rate (SFR) and the stellar mass, i.e. the Mai...
We study the history from z similar to 2 to z similar to 0 of the stellar mass assembly of quiescent...
Context. Most of the massive star-forming galaxies are found to have “inside-out” stellar mass growt...
We present an analysis of the spatial distribution of star formation in a sample of 60 visually iden...
We present an analysis of the spatial distribution of star formation in a sample of 60 visually iden...
International audienceUsing data from four deep fields (COSMOS, AEGIS, ECDFS, and CDFN), we study th...
The assembly of galaxies can be described by the distribution of their star formation as a function ...
Near infrared slitless spectroscopy with the Wide Field Camera 3, on board the Hubble Space Telescop...
For a mass-selected sample of 66544 galaxies with photometric redshifts (z phot) from the Cosmic Evo...
The assembly of galaxies can be described by the distribution of their star formation as a function ...
We present an analysis of the spatial distribution of star formation in a sample of 60 visually iden...
International audienceHigh-resolution multi-wavelength photometry is crucial to explore the spatial ...
High-resolution multi-wavelength photometry is crucial to explore the spatial distribution of star f...
Using spatially resolved Hα emission line maps of star-forming galaxies, we study the spatial distri...
We perform the first spatially-resolved stellar population study of galaxies in the early universe z...
We investigate the relation between the star formation rate (SFR) and the stellar mass, i.e. the Mai...
We study the history from z similar to 2 to z similar to 0 of the stellar mass assembly of quiescent...
Context. Most of the massive star-forming galaxies are found to have “inside-out” stellar mass growt...
We present an analysis of the spatial distribution of star formation in a sample of 60 visually iden...
We present an analysis of the spatial distribution of star formation in a sample of 60 visually iden...
International audienceUsing data from four deep fields (COSMOS, AEGIS, ECDFS, and CDFN), we study th...
The assembly of galaxies can be described by the distribution of their star formation as a function ...
Near infrared slitless spectroscopy with the Wide Field Camera 3, on board the Hubble Space Telescop...
For a mass-selected sample of 66544 galaxies with photometric redshifts (z phot) from the Cosmic Evo...
The assembly of galaxies can be described by the distribution of their star formation as a function ...
We present an analysis of the spatial distribution of star formation in a sample of 60 visually iden...