Tipo de publicación: Con árbitro

  • Publicación
    A decade of near-infrared variability in NGC4388: insights into the AGN structure
    Variability studies have proven to be a powerful diagnostic tool for understanding the physics and properties of active galactic nuclei (AGNs). They provide...
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    A Decade of the Moderate Resolution Imaging Spectroradiometer: Is a Solar-Cloud Link Detectable?
    Not Available
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    A DECam view of the diffuse dwarf galaxy Crater II - Variable stars
    Time series observations of a single dithered field centred on the diffuse dwarf satellite galaxy Crater II were obtained with the Dark Energy Camera (DECam) at...
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    A DECam view of the diffuse dwarf galaxy Crater II: the colour-magnitude diagram
    We present a deep Blanco/DECam colour-magnitude diagram (CMD) for the large but very diffuse Milky Way satellite dwarf galaxy Crater II. The CMD shows only old...
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    A deep learning approach to infer galaxy cluster masses from Planck Compton-y parameter maps
    Galaxy clusters are useful laboratories to investigate the evolution of the Universe, and accurate measurement of their total masses allows us to constrain...
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    A deep learning approach to test the small-scale galaxy morphology and its relationship with star formation activity in hydrodynamical simulations
    Hydrodynamical simulations of galaxy formation and evolution attempt to fully model the physics that shapes galaxies. The agreement between the morphology of...
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    A deep look at the nuclear region of UGC 5101 through high angular resolution mid-IR data with GTC/CanariCam
    We present an analysis of the nuclear infrared (IR, 1.6-18 μm) emission of the ultraluminous IR galaxy UGC 5101 to derive the properties of its active galactic...
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    A deep look into the core of young clusters. II. λ-Orionis
    Context: Over the past years, the λ-Orionis cluster has been a prime location for the study of young very low mass stars, substellar and isolated planetary mass...
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    A deep look into the cores of young clusters. I. σ-Orionis
    Context: Nearby young clusters are privileged places to study the star formation history. Over the last decade, the σ-Orionis cluster has been a prime location...