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

  • Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
    Recent observations have detected galaxies at high-redshift z∼ 6{--}11, and revealed the diversity of their physical properties, from normal star-forming galaxies to starburst galaxies. To understand the properties of these observed galaxies, it is crucial to understand the star formation (SF) history of high-redshift galaxies under the influence
    Yajima, H. et al.

    Fecha de publicación:

    9
    2017
    Número de citas
    38
  • H-ATLAS: a candidate high redshift cluster/protocluster of star-forming galaxies
    We investigate the region around the Planck-detected z = 3.26 gravitationally lensed galaxy HATLAS J114637.9-001132 (hereinafter HATLAS12-00) using both archival Herschel data from the H-ATLAS survey and using submm data obtained with both LABOCA and SCUBA2. The lensed source is found to be surrounded by a strong overdensity of both Herschel-SPIRE
    Clements, D. L. et al.

    Fecha de publicación:

    9
    2016
    Número de citas
    32
  • HADES RV Programme with HARPS-N at TNG. V. A super-Earth on the inner edge of the habitable zone of the nearby M dwarf GJ 625
    We report the discovery of a super-Earth orbiting at the inner edge of the habitable zone of the star GJ 625 based on the analysis of the radial-velocity (RV) time series from the HARPS-N spectrograph, consisting of 151 HARPS-N measurements taken over 3.5 yr. GJ 625 b is a planet with a minimum mass Msini of 2.82 ± 0.51 M⊕ with an orbital period of
    Suárez Mascareño, A. et al.

    Fecha de publicación:

    9
    2017
    Número de citas
    29
  • HARPS Observes the Earth Transiting the Sun — A Method to Study Exoplanet Atmospheres Using Precision Spectroscopy on Large Ground-based Telescopes
    Exoplanetary transits offer the opportunity to measure the transmission of long, tangential pathlengths through their atmospheres. Since the fraction of the observed stellar light taking these paths is very small, transit photometric and spectrophotometric measurements of light curves require very high levels of measurement stability, favouring the
    Yan, F. et al.

    Fecha de publicación:

    9
    2015
    Número de citas
    0
  • HAZEL: HAnle and ZEeman Light
    A big challenge in solar and stellar physics in the coming years will be to decipher the magnetism of the solar outer atmosphere (chromosphere and corona) along with its dynamic coupling with the magnetic fields of the underlying photosphere. To this end, it is important to develop rigorous diagnostic tools for the physical interpretation of
    Asensio Ramos, Andrés et al.

    Fecha de publicación:

    9
    2011
    Número de citas
    2
  • HD 17156 transit photometry & radial velocities (Barbieri+, 2009)
    This table contains the photometric time serie obtained for a series of transits of the planet HD 17156b. The first column gives the date as Barycentric Julian Days (BJD), the second one gives the flux normalized to the out-of-transit average value, and the third one gives the Identification code of each observation. (2 data files).
    Barbieri, M. et al.

    Fecha de publicación:

    9
    2009
    Número de citas
    0