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

  • A map-making algorithm for the QUIJOTE CMB experiment
    In the last years we obtained a very detailed picture of the Primordial Universe by, among other means, measuring the intensity and the polarization of the Cosmic Microwave Background (CMB). With the last space missions WMAP and Planck we entered in the precision Cosmology era. Nowadays, ground-based experiments are measuring the sky looking for
    Guidi, F. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    0
  • A collection of model stellar spectra for spectral types B to early-M
    Context. Models of stellar spectra are necessary for interpreting light from individual stars, planets, integrated stellar populations, nebulae, and the interstellar medium. Aims: We provide a comprehensive and homogeneous collection of synthetic spectra for a wide range of atmospheric parameters and chemical compositions. Methods: We compile
    Allende Prieto, C. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    72
  • A clockwork solution to the flavor puzzle
    We introduce a set of clockwork models of flavor that can naturally explain the large hierarchies of the Standard Model quark masses and mixing angles. Since the clockwork only contains chains of new vector-like fermions without any other dynamical fields, the flavor constraints allow for relatively light new physics scale. For two benchmarks with
    Alonso, R. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    45
  • 3D non-LTE corrections for Li abundance and 6Li/7Li isotopic ratio in solar-type stars. I. Application to HD 207129 and HD 95456
    Context. Convective motions in solar-type stellar atmospheres induce Doppler shifts that affect the strengths and shapes of spectral absorption lines and create slightly asymmetric line profiles. One-dimensional (1D) local thermodynamic equilibrium (LTE) studies of elemental abundances are not able to reproduce this phenomenon, which becomes
    Harutyunyan, G. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    25
  • 3C 17: The BCG of a Galaxy Cluster at z = 0.22
    Gemini Multi Object Spectrograph medium-resolution spectra and photometric data of 39 objects in the field of the radio galaxy 3C 17 are presented. Based on the new data, a previously uncataloged cluster of galaxies is identified at a mean redshift of z = 0.220 ± 0.003, a projected virial radius of 0.37 Mpc, and a velocity dispersion of σ v = 821 ±
    Madrid, Juan P. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    12
  • UNVEILING THE NATURE OF THE MOST LUMINOUS GALAXIES AT THE COSMIC NOON
    This thesis focus on understanding the physical properties of galaxies at redshifts 2.3 < z < 3.3, a time period called Cosmic Noon when galaxies were actively forming stars and evolving rapidly. The work involves the study of different galaxy populations, from young Lyα emitters (LAEs) and Lyman break galaxies (LBGs), to more evolved, and very
    Rui José Marques Coelho Chaves

    Fecha de publicación:

    9
    2018