Astrofísicas: Cosmología

  • Publicación
    Extended dark energy analysis using DESI DR2 BAO measurements
    We conduct an extended analysis of dark energy constraints, in support of the findings of the Dark Energy Spectroscopic Instrument (DESI) second data release...
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    Extracting cosmological information from the angular power spectrum of the 2MASS Photometric Redshift catalogue
    Using the almost all-sky 2MASS Photometric Redshift catalogue (2MPZ) we perform for the first time a tomographic analysis of galaxy angular clustering in the...
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    Extragalactic Archaeology: The Assembly History of Galaxies from Dynamical and Stellar Population Models
    In this review, we show how combining dynamical and stellar population models with integral field spectroscopic data of nearby galaxies enables uncovering their...
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    Extragalactic science with EMIR-GTC
    EMIR is a wide-field, near-IR spectrograph currently under development for the Nasmyth focus of the Spanish 10.4m GTC at Canary Islands. EMIR will provide...
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    Fast simulation mapping: From standard to modified gravity cosmologies using the bias assignment method
    Context. We assess the effectiveness of a non-parametric bias model in generating mock halo catalogues for modified gravity (MG) cosmologies, relying on the...
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    Finding galaxy clusters using Voronoi tessellations
    We present an objective and automated procedure for detecting clusters of galaxies in imaging galaxy surveys. Our Voronoi Galaxy Cluster Finder (VGCF) uses...
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    First Cosmology Results using Supernovae Ia from the Dark Energy Survey: Survey Overview, Performance, and Supernova Spectroscopy
    We present details on the observing strategy, data-processing techniques, and spectroscopic targeting algorithms for the first three years of operation for the...
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    First results from the Very Small Array - I. Observational methods
    The Very Small Array (VSA) is a synthesis telescope designed to image faint structures in the cosmic microwave background on degree and sub-degree angular...
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    First results from the Very Small Array - II. Observations of the cosmic microwave background
    We have observed the cosmic microwave background (CMB) temperature fluctuations in eight fields covering three separated areas of sky with the Very Small Array...