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

  • Errata
    Erratum: The Herschel PEP/HerMES Luminosity Function - I. Probing the Evolution of PACS selected Galaxies to z ≃ 4
    Not Available
    Gruppioni, C. et al.

    Fecha de publicación:

    12
    2013
    Bibcode
    2013MNRAS.436.2875G
    Número de citas
    10
  • Errata
    Erratum: The properties of the stellar populations in ULIRGs - II. Star formation histories and evolution
    Not Available
    Rodríguez Zaurín, J. et al.

    Fecha de publicación:

    12
    2010
    Bibcode
    2010MNRAS.409.1728R
    Número de citas
    0
  • Errata
    Erratum: ``H I in the Shell Elliptical Galaxy NGC 3656'' [Astron. J. 122, 1758 (2001)]
    As the result of an editorial oversight, the following two works were misattributed in the references:Schweizer, F. 1998, in Galaxies: Interactions and Induced Star Formation, ed. D. Friedli, L. Martinet, & D. Pfenniger (Berlin: Springer), 105Sparke, L. S. 1996, ApJ, 473, 810The publisher regrets the error.
    Balcells, Marc et al.

    Fecha de publicación:

    12
    2001
    Bibcode
    2001AJ....122.3508B
    Número de citas
    1
  • Con árbitro
    ERRATUM: “Probing the deep end of the Milky Way with Kepler: Asteroseismic Analysis of 854 faint Red Giants misclassified as Cool Dwarfs” (2016, ApJ, 827, 50)
    Not Available
    Salabert, D. et al.

    Fecha de publicación:

    12
    2016
    Bibcode
    2016ApJ...833..294M
    Número de citas
    4
  • Con árbitro
    Estimate of the Accretion Disk Size in the Gravitationally Lensed Quasar HE 0435–1223 Using Microlensing Magnification Statistics
    We present a measurement of the accretion disk size of the quadruple lensed quasar HE 0435–1223 from well-sampled 13-year COSMOGRAIL optical light curves. Using accurate time delays for the images A, B, C, and D, we modeled and removed the intrinsic quasar variability, and found microlensing events of amplitude up to 0.6, 0.4, and 0.5 mag in the
    Fian, C. et al.

    Fecha de publicación:

    12
    2018
    Bibcode
    2018ApJ...869..132F
    Número de citas
    14
  • Con árbitro
    Estimating the Reliability of Digital Data Acquisition in Cultural Astronomy: The Case of Roman North Africa
    Digital tools are increasingly used in cultural astronomy, so that it is now more important than ever to assess their precision and reliability, and to identify what uncertainties they may introduce. The present work aims to address these issues by comparing a dataset of orientations of Roman cities in the Iberian Peninsula measured in situ with
    Andrea Rodríguez-Antón, A. et al.

    Fecha de publicación:

    12
    2017