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

  • Perturbation theory for modeling galaxy bias: Validation with simulations of the Dark Energy Survey
    We describe perturbation theory (PT) models of galaxy bias for applications to photometric galaxy surveys. We model the galaxy-galaxy and galaxy-matter correlation functions in configuration space and validate against measurements from mock catalogs designed for the Dark Energy Survey (DES). We find that an effective PT model with five galaxy bias
    Pandey, S. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    34
  • Separation between RR Lyrae and type II Cepheids and their importance for a distance determination: the case of omega Cen
    The separation between RR Lyrae (RRLs) and type II Cepheid (T2Cs) variables based on their period is debated. Both types of variable stars are distance indicators, and we aim to promote the use of T2Cs as distance indicators in synergy with RRLs. We adopted new and existing optical and near-infrared (NIR) photometry of ω Cen to investigate several
    Braga, V. F. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    21
  • The EDGE-CALIFA survey: exploring the role of molecular gas on galaxy star formation quenching
    Understanding how galaxies cease to form stars represents an outstanding challenge for galaxy evolution theories. This process of "star formation quenching" has been related to various causes, including active galactic nuclei activity, the influence of large-scale dynamics, and the environment in which galaxies live. In this paper, we present the
    Colombo, D. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    36
  • The kinematics of young and old stellar populations in nuclear rings of MUSE TIMER galaxies
    Context. Studying the stellar kinematics of galaxies is a key tool in the reconstruction of their evolution. However, the current measurements of the stellar kinematics are complicated by several factors, including dust extinction and the presence of multiple stellar populations. Aims: We use integral field spectroscopic data of four galaxies from
    Rosado-Belza, D. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    7
  • A comprehensive study of the WASP-74 planetary system
    In this work, we present new transit observations of the hot Jupiter WASP-74 b using the high-resolution spectrograph HARPS-N and the multi-color simultaneous imager MuSCAT2. The new data allow us to refine the orbital properties of the planet, the physical parameters of the host star, and reveal some properties about the planet's atmosphere using
    Luque, Rafael

    Fecha de publicación:

    9
    2020
    Número de citas
    0
  • Basaltic material across the Main Asteroid Belt
    The inner main belt asteroid (4) Vesta, with a diameter of about 525 km, is the largest differentiated asteroid showing a basaltic crust [1]. The collisional family of Vesta includes more than 15,000 known members [2] and it is considered the main source of basaltic material. The results found by the Dawn mission support the hypothesis that this
    Alexandru Mansour, Jad et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    0