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

  • Con árbitro
    The UKIRT Infrared Deep Sky Survey (UKIDSS)
    We describe the goals, design, implementation, and initial progress of the UKIRT Infrared Deep Sky Survey (UKIDSS), a seven-year sky survey which began in 2005 May. UKIDSS is being carried out using the UKIRT Wide Field Camera (WFCAM), which has the largest étendue of any infrared astronomical instrument to date. It is a portfolio of five survey
    Lawrence, A. et al.

    Fecha de publicación:

    8
    2007
    Bibcode
    2007MNRAS.379.1599L
    Número de citas
    1000
  • Con árbitro
    The substellar mass function in σ Orionis. II. Optical, near-infrared and IRAC/Spitzer photometry of young cluster brown dwarfs and planetary-mass objects
    Aims:We investigate the mass function in the substellar domain down to a few Jupiter masses in the young σ Orionis open cluster (3±2 Ma, d = 360^+70_-60 pc). Methods: We have performed a deep IJ-band search, covering an area of 790 arcmin2 close to the cluster centre. This survey was complemented with an infrared follow-up in the HK_s- and Spitzer
    Caballero, J. A. et al.

    Fecha de publicación:

    8
    2007
    Bibcode
    2007A&A...470..903C
    Número de citas
    121
  • Sin árbitro
    The Star Formation History of Phoenix Dwarf Galaxy using IAC-pop Algorithm
    Not Available
    Hidalgo, Sebastian L. et al.

    Fecha de publicación:

    8
    2007
    Bibcode
    2007IAUS..241..345H
    Número de citas
    0
  • Sin árbitro
    The Star Formation History in a SMC field: IAC-star/IAC-pop at work
    We present a progress report of a project to study the quantitative star formation history (SFH) in different parts of the Small Magellanic Cloud (SMC). We use the information in [(B-R), R] color-magnitude diagrams (CMDs), which reach down to the oldest main-sequence turnoffs and allow us to retrieve the SFH in detail. We show the first results of
    Noël, Noelia E. D. et al.

    Fecha de publicación:

    8
    2007
    Bibcode
    2007IAUS..241..373N
    Número de citas
    1