Astrophysical: Galaxies

  • Publication
    Spatially resolved dust properties over 50 kpc in a hyperluminous galaxy merger at z = 4.6
    We present spatially resolved dust-continuum ALMA observations from rest frame ∼60 to ∼600 μm (bands 3–10) of the hyperluminous hot dust-obscured galaxy (hot...
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    Spatially resolved evidence of the impact of quasar-driven outflows on recent star formation: the case of Mrk 34
    We present the results of our spatially resolved investigation into the interplay between the ages of the stellar populations and the kinematics of the warm...
  • Publication
    Spatially resolved LMC star formation history - I. Outside in evolution of the outer LMC disc
    We study the evolution of three fields in the outer Large Magellanic Cloud (LMC) disc (Rgc = 3.5-6.2 kpc). Their star formation history indicates a stellar...
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    Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
    We present a framework to build realistic mock spectroscopic observations for state-of-the-art hydrodynamical simulations, using high spectral resolution...
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    Spatially resolved properties of the ionized gas in the H II galaxy J084220+115000
    We present a spatially resolved spectroscopic study for the metal poor H II galaxy J084220+115000 using MEGARA Integral Field Unit observations at the Gran...
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    Spatially resolved self-consistent spectral modelling of jellyfish galaxies from MUSE with FADO: trends with mass and stripping intensity
    We present a spatially resolved stellar population analysis of 61 jellyfish galaxies and 47 control galaxies observed with ESO/MUSE attempting to understand the...
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    Spatially Resolved Spectroscopy and Chemical History of Star-forming Galaxies in the Hercules Cluster: The Effects of the Environment
    Spatially resolved spectroscopy has been obtained for a sample of 27 star-forming (SF) galaxies selected from our deep Hα survey of the Hercules cluster. We...
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    Spatially Resolved Star Formation Main Sequence of Galaxies
    The relation known as Star Formation Main Sequence (SFMS) of galaxies is defined in terms of stellar mass and star formation rate. This approximately linear...
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    Spatially Resolved Star Formation Main Sequence of Galaxies in the CALIFA Survey
    The “main sequence of galaxies”—defined in terms of the total star formation rate ψ versus the total stellar mass M *—is a well-studied tight relation that has...