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

  • On the building blocks of the M31 and Milky Way halos
    We discuss the formation of the halo of M31 and the Milky Way as traced by the population of RR Lyrae stars, in comparison with the population of such stars preent in satellite dwarf galaxies. We find that both halos and the massive dwarf host a population of high amplitude short period RRab stars, absent in low-mass dwarfs. These stars are
    Monelli, M.

    Fecha de publicación:

    9
    2017
    Número de citas
    0
  • Observational constraints to boxy/peanut bulge formation time
    Boxy/peanut bulges are considered to be part of the same stellar structure as bars and both could be linked through the buckling instability. The Milky Way is our closest example. The goal of this Letter is to determine if the mass assembly of the different components leaves an imprint in their stellar populations allowing the estimation the time
    Pérez, I. et al.

    Fecha de publicación:

    9
    2017
    Número de citas
    21
  • Near-InfraRed Planet Searcher to Join HARPS on the ESO 3.6-metre Telescope
    The Near-InfraRed Planet Searcher (NIRPS) is a new ultra-stable infrared (YJH) spectrograph that will be installed on ESO's 3.6-metre Telescope in La Silla, Chile. Aiming to achieve a precision of 1 m s-1, NIRPS is designed to find rocky planets orbiting M dwarfs, and will operate together with the High Accuracy Radial velocity Planet Searcher
    Bouchy, F. et al.

    Fecha de publicación:

    9
    2017
    Número de citas
    65
  • Meteor studies in the framework of the JEM-EUSO program
    We summarize the state of the art of a program of UV observations from space of meteor phenomena, a secondary objective of the JEM-EUSO international collaboration. Our preliminary analysis indicates that JEM-EUSO, taking advantage of its large FOV and good sensitivity, should be able to detect meteors down to absolute magnitude close to 7. This
    Abdellaoui, G. et al.

    Fecha de publicación:

    9
    2017
    Número de citas
    19
  • Measurements of the charm jet cross section and nuclear modification factor in pPb collisions at √{sNN} = 5.02 TeV
    The CMS Collaboration presents the first measurement of the differential cross section of jets from charm quarks produced in proton-lead (pPb) collisions at a nucleon-nucleon center-of-mass energy of √{sNN} = 5.02TeV, as well as results from charm quark jets in proton-proton (pp) collisions at √{ s} = 2.76 and 5.02TeV. By comparing the yields of
    Sirunyan, A. M. et al.

    Fecha de publicación:

    9
    2017
    Número de citas
    24
  • Measurement of the t\overline{t} production cross section using events with one lepton and at least one jet in pp collisions at √{s}=13 TeV
    A measurement of the t\overline{t} production cross section at √{s}=13 TeV is presented using proton-proton collisions, corresponding to an integrated luminosity of 2.2 fb-1, collected with the CMS detector at the LHC. Final states with one isolated charged lepton (electron or muon) and at least one jet are selected and categorized according to the
    Sirunyan, A. M. et al.

    Fecha de publicación:

    9
    2017
    Número de citas
    23