Tipo de publicación: Con árbitro

  • Publicación
    Expectations and Limits to Synthesize Nuclei with Z ≥ 120
    In order to explore the possibilities to synthesize the new superheavy elements with Z=120, 122, 124, 126 some hot-fusion (mass asymmetric) reactions and cold...
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    Expectations of the Size Evolution of Massive Galaxies at 3 ≤ z ≤ 6 from the TNG50 Simulation: The CEERS/JWST View
    We present a catalog of about 25,000 images of massive (M ⋆ ≥ 10 9 M ⊙) galaxies at redshifts 3 ≤ z ≤ 6 from the TNG50 cosmological simulation, tailored for...
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    Expected Number of Massive Galaxy Relics in the Present Day Universe
    The number of present day massive galaxies that have survived untouched since their formation at high-z is an important observational constraint to the...
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    Expected spectral characteristics of (101955) Bennu and (162173) Ryugu, targets of the OSIRIS-REx and Hayabusa2 missions
    NASA's OSIRIS-REx and JAXA's Hayabusa2 sample-return missions are currently on their way to encounter primitive near-Earth asteroids (101955) Bennu and (162173)...
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    Experimental measurement of the quality factor of a Fabry-Pérot open-cavity axion haloscope
    The axion is a hypothetical boson arising from the most natural solution to the problem of charge and parity symmetry in the strong nuclear force. Moreover...
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    Experimental validation of Lyot stop apodization in ground-based coronagraphy
    We show that the use of apodizing functions at the coronagraph Lyot plane may be useful for improving the image contrast of ground-based coronagraphs. An...
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    Explaining the chemical trajectories of accreted and in-situ halo stars of the Milky Way
    The Milky Way underwent its last significant merger ten billion years ago, when the Gaia-Enceladus-Sausage (GES) was accreted. Accreted GES stars and progenitor...
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    Explaining the Galactic Interstellar Dust Grain Size Distribution Function
    We present here a new theoretical model designed to explain the interstellar dust grain size distribution function (IDGSDF), and compare its results with...
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    Explaining the Mysterious Age Gap of Globular Clusters in the Large Magellanic Cloud
    The Large Magellanic Cloud (LMC) has a unique cluster formation history in that nearly all of its globular clusters were formed either ~13 Gyr ago or less than...