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

  • Swift J1910.2-0546/MAXI J1910-057: Optical Imaging and Spectroscopy with the Liverpool Telescope
    We report on optical spectroscopy of the high-energy transient Swift J1910.2-0546 / MAXI 1910-057 (ATel #4139; #4140; #4171; #4195; #4198) using the 2m Liverpool Telescope on La Palma and the FRODOSPEC spectrograph. On 2012 June 18 (01:25 UTC) we obtained 1500s exposures simultaneously in the red (5700-8050A at 0.59A/pixel) and blue (3800-5150A at
    Charles, Phil et al.

    Fecha de publicación:

    6
    2012
    Número de citas
    7
  • Structure and dynamics of galaxies with a low surface-brightness disc - II. Stellar populations of bulges
    We present the radial profiles of the Hβ, Mg and Fe line-strength indices for a sample of eight spiral galaxies with a low-surface-brightness stellar disc and a bulge. The correlations between the central values of the line-strength indices and velocity dispersion are consistent with those known for early-type galaxies and bulges of high-surface
    Morelli, L. et al.

    Fecha de publicación:

    6
    2012
    Número de citas
    38
  • SPIRE (f250um>17.4mJy) GOODS-N galaxies (Symeonidis+, 2011)
    The IR data come from the Herschel/SPIRE Science Demonstration Phase (SDP) observations of the Great Observatories Origins Deep Survey (GOODS)-North, taken as part of the Herschel Multi-tiered Extragalactic Survey (HerMES) guaranteed-time key programme. (1 data file).
    Symeonidis, M. et al.

    Fecha de publicación:

    6
    2012
    Número de citas
    0
  • Satellites around Massive Galaxies Since z ~ 2: Confronting the Millennium Simulation with Observations
    Minor merging has been postulated as the most likely evolutionary path to produce the increase in size and mass observed in the massive galaxies since z ~ 2. In this Letter, we directly test this hypothesis, comparing the population of satellites around massive galaxies in cosmological simulations versus the observations. We use state-of-the-art
    Quilis, Vicent et al.

    Fecha de publicación:

    6
    2012
    Número de citas
    22