About this community

Wide range of research programmes linked to experimental and instrumental programmes at the cutting edge of astronomical technology

The wide range of research programmes carried out by the group are centred on four major areas each linked to experimental and instrumental programmes which are at the cutting edge of astronomical technology.

These activities are supported by theoretical studies, particularly in the area of fundamental physics applications in Relativity and Cosmology, as well as modelling and simulation of astronomical phenomena.

Note from the editors to depositors: Collections within this community can be set-up, structured and named according to your specific requirements. If you have suggestions, please contact us.

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Recent Submissions

  • Characterization of star-forming dwarf galaxies at 0.1 ≲ z ≲ 0.9 in VUDS: Probing the low-mass end of the mass-metallicity relation 

    Calabrò, A; Amorín, Ricardo Oscar; Fontana, A; Pérez-Montero, E; Lemaux, BC; Ribeiro, B; Bardelli, S et al. (2017-05-01)
    © 2017 ESO. Context. The study of statistically significant samples of star-forming dwarf galaxies (SFDGs) at different cosmic epochs is essential for the detailed understanding of galaxy assembly and chemical evolution. ...
  • The supermassive black hole coincident with the luminous transient ASASSN-15lh 

    Krühler, T; Fraser, M; Leloudas, G; Schulze, S; Stone, NC; Van Velzen, S; Amorin, Ricardo Oscar et al. (2018-02-01)
  • The VIMOS Ultra-Deep Survey: A major merger origin for the high fraction of galaxies at 2 < z < 6 with two bright clumps 

    Ribeiro, B; Le Fèvre, O; Cassata, P; Garilli, B; Lemaux, BC; Maccagni, D; Schaerer, D et al. (2017-12-01)
    © 2017 ESO. The properties of stellar clumps in star-forming galaxies and their evolution over the redshift range 2 ≲ z ≲ 6 are presented and discussed in the context of the build-up of massive galaxies at early cosmic ...
  • The MUSE view of the host galaxy of GRB 100316D 

    Izzo, L; Thäone, CC; Schulze, S; Mehner, A; Flores, H; Cano, Z; de Ugarte Postigo, A et al. (2017-12-01)
    The low distance, z = 0.0591, of GRB 100316D and its association with SN 2010bh represent two important motivations for studying this host galaxy and the GRB’s immediate environment with the integral field spectrographs ...

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