Tipo de publicación: Con árbitro

  • Publicación
    Damping of magnetohydrodynamic waves by resonant absorption in the solar atmosphere
    Not Available
  • Publicación
    Damping of prominence longitudinal oscillations due to mass accretion
    We study the damping of longitudinal oscillations of a prominence thread caused by the mass accretion. We suggested a simple model describing this phenomenon...
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    Dark Energy Survey Deep Field photometric redshift performance and training incompleteness assessment
    Context. The determination of accurate photometric redshifts (photo-zs) in large imaging galaxy surveys is key for cosmological studies. One of the most common...
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    Dark Energy Survey Y3 results: blending shear and redshift biases in image simulations
    As the statistical power of galaxy weak lensing reaches per cent level precision, large, realistic, and robust simulations are required to calibrate...
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    Dark energy survey year 1 results: Constraining baryonic physics in the Universe
    Measurements of large-scale structure are interpreted using theoretical predictions for the matter distribution, including potential impacts of baryonic physics...
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    Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations
    We present the first joint analysis of cluster abundances and auto or cross-correlations of three cosmic tracer fields: galaxy density, weak gravitational...
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    Dark Energy Survey Year 1 results: the lensing imprint of cosmic voids on the cosmic microwave background
    Cosmic voids gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint on degree scales. We use the simulated CMB...
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    Dark Energy Survey year 1 results: the relationship between mass and light around cosmic voids
    What are the mass and galaxy profiles of cosmic voids? In this paper, we use two methods to extract voids in the Dark Energy Survey (DES) Year 1 redMaGiC galaxy...
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    Dark Energy Survey Year 3 results: A 2.7% measurement of baryon acoustic oscillation distance scale at redshift 0.835
    We present angular diameter measurements obtained by measuring the position of baryon acoustic oscillations (BAO) in an optimized sample of galaxies from the...