Astrophysical: Star formation

  • Publication
    The effect of environment on star forming galaxies at redshift 1 First insight from PACS (Corrigendum)
    Not Available
  • Publication
    The effect of environment on star forming galaxies at redshift. I. First insight from PACS
    We use deep 70, 100 and 160 μm observations taken with PACS, the Photodetector Array Camera and Spectrometer on board of Herschel, as part of the PACS...
  • Publication
    The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
    Recent observational and theoretical studies indicate that the stellar initial mass function (IMF) varies systematically with the environment (star formation...
  • Publication
    The ELMER Detection Subsystem
    ELMER is a multi-purpose instrument for the GTC designed for both, imaging and spectroscopy in the visible range. The detection subsystem consists of a single...
  • Publication
    The embedded cluster IRAS17136 - 3617 associated with the nebulosity GM24
    Radio, infrared, and optical observations of the embedded infrared cluster IRAS17136 - 3617 are reviewed. The cluster consists of more than 25 stars with a...
  • Publication
    The EROs at z < 1.5 in the Groth-Westphal field of the GOYA survey
    The study of the Extremly Red Objects (EROs), is the importance for setting constraints on the first epoch of massive galaxy formation, for exploring the...
  • Publication
    The evolution of compact massive quiescent and star-forming galaxies derived from the R<SUB>e</SUB>-R<SUB>h</SUB> and M<SUB>star</SUB>-M<SUB>h</SUB> relations
    The mean size (effective radius R e) of massive galaxies (MGs; M star > 10 11.2M ⊙) is observed to increase steadily with cosmic time. It is still unclear...
  • Publication
    The evolution of quiescent galaxies at high redshifts (z≥ 1.4)
    The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an effective area of ˜1.7 deg2 in the COSMOS field. Galaxies...
  • Publication
    The evolution of rest-frame UV properties, Ly α EWs, and the SFR-stellar mass relation at z ̃ 2-6 for SC4K LAEs
    We explore deep rest-frame UV to FIR data in the COSMOS field to measure the individual spectral energy distributions (SED) of the ̃4000 SC4K (Sobral et al.)...