Tipo de publicación: Con árbitro

  • Publicación
    The impact from survey depth and resolution on the morphological classification of galaxies
    We consistently analyse for the first time the impact of survey depth and spatial resolution on the most used morphological parameters for classifying galaxies...
  • Publicación
    The impact of a non-universal Initial Mass Function on the star formation histories of early-type galaxies
    Recent results on the non-universality of the Initial Mass Function (IMF) have shown strong evidence of IMF variations with galaxy velocity dispersion, with a...
  • Publicación
    The Impact of Angle-dependent Partial Frequency Redistribution on the Scattering Polarization of the Solar Na I D Lines
    The long-standing paradox of the linear polarization signal of the Na I D 1 line was recently resolved by accounting for the atom's hyperfine structure and the...
  • Publicación
    The Impact of Bars on Disk Breaks as Probed by S4G Imaging
    We have analyzed the radial distribution of old stars in a sample of 218 nearby face-on disks, using deep 3.6 μm images from the Spitzer Survey of Stellar...
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    The impact of baryons on the spins and shapes of dark matter haloes
    We use numerical simulations to investigate how the statistical properties of dark matter (DM) haloes are affected by the baryonic processes associated with...
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    The impact of different physical processes on the statistics of Lyman-limit and damped Lyman α absorbers
    We compute the z = 3 neutral hydrogen column density distribution function f(NHI) for 19 simulations drawn from the Overwhelmingly Large Simulations project...
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    The Impact of Enhanced He and CNONa Abundances on Globular Cluster Relative Age-Dating Methods
    The impact that unrecognized differences in the chemical patterns of Galactic globular clusters (GGCs) have on their relative age determinations is studied. The...
  • Publicación
    The Impact of Evolving Infrared Spectral Energy Distributions of Galaxies on Star Formation Rate Estimates
    We combine Herschel-Photodetector Array Camera and Spectrometer (PACS) data from the PACS Evolutionary Probe (PEP) program with Spitzer 24 μm and 16 μm...
  • Publicación
    The impact of filaments on dwarf galaxy properties in the Auriga simulations
    With a hydrodynamical simulation using a simple galaxy formation model without taking into account feedback, our previous work has shown that dense and massive...