Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • YORP Effect on Asteroid 162173 Ryugu: Implications for the Dynamical History
    Asteroid 162173 Ryugu is a carbonaceous asteroid that was visited by Japan's Hayabusa2 spacecraft in 2018. The formation mechanism of the "spinning-top" shape of Ryugu is a vital clue to the dynamical history of the near-Earth asteroid. In this study, we address the long-term evolution of its spin state induced by the Yarkovsky-O'Keefe-Radzievskii
    Kanamaru, Masanori et al.

    Fecha de publicación:

    12
    2021
    Número de citas
    6
  • 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 observational systematics, especially given the increased importance of object blending as survey depths increase. To capture the coupled effects of blending in both shear and photometric redshift
    MacCrann, N. et al.

    Fecha de publicación:

    1
    2022
    Número de citas
    89
  • Dark Energy Survey Year 3 Results: Deep Field optical + near-infrared images and catalogue
    We describe the Dark Energy Survey (DES) Deep Fields, a set of images and associated multiwavelength catalogue (ugrizJHKs) built from Dark Energy Camera (DECam) and Visible and Infrared Survey Telescope for Astronomy (VISTA) data. The DES Deep Fields comprise 11 fields (10 DES supernova fields plus COSMOS), with a total area of ~30 sq. deg. in
    Hartley, W. G. et al.

    Fecha de publicación:

    1
    2022
    Número de citas
    58
  • Dark Energy Survey Year 3 results: galaxy sample for BAO measurement
    In this paper, we present and validate the galaxy sample used for the analysis of the baryon acoustic oscillation (BAO) signal in the Dark Energy Survey (DES) Y3 data. The definition is based on a colour and redshift-dependent magnitude cut optimized to select galaxies at redshifts higher than 0.5, while ensuring a high-quality determination. The
    Carnero Rosell, A. et al.

    Fecha de publicación:

    1
    2022
  • Dark Energy Survey Year 3 results: galaxy-halo connection from galaxy-galaxy lensing
    Galaxy-galaxy lensing is a powerful probe of the connection between galaxies and their host dark matter haloes, which is important both for galaxy evolution and cosmology. We extend the measurement and modelling of the galaxy-galaxy lensing signal in the recent Dark Energy Survey Year 3 cosmology analysis to the highly non-linear scales (~100 kpc)
    Zacharegkas, G. et al.

    Fecha de publicación:

    1
    2022
    Número de citas
    29
  • FOREVER22: galaxy formation in protocluster regions
    We present results from a new cosmological hydrodynamics simulation campaign of protocluster (PC) regions, FOREVER22: FORmation and EVolution of galaxies in Extremely overdense Regions motivated by SSA22. The simulations cover a wide range of cosmological scales using three different zoom set-ups in a parent volume of $(714.2~\rm cMpc)^{3}$: PCR
    Yajima, Hidenobu et al.

    Fecha de publicación:

    1
    2022
    Número de citas
    31