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

  • Early science with the LMT: molecular torus in UGC 5101
    As part of the Early Science Large Millimeter Telescope projects, we report the detection of nine double-peaked molecular lines, produced by a rotating molecular torus, in the ultraluminous infrared galaxies (ULIRG) - Compton-thick active galactic nuclei (AGN) galaxy UGC 5101. The double-peaked lines we report correspond to molecular transitions of
    Cruz-González, I. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    5
  • Dust Reverberation Mapping in Distant Quasars from Optical and Mid-infrared Imaging Surveys
    The size of the dust torus in active galactic nuclei (AGNs) and their high-luminosity counterparts, quasars, can be inferred from the time delay between UV/optical accretion disk continuum variability and the response in the mid-infrared (MIR) torus emission. This dust reverberation mapping (RM) technique has been successfully applied to ∼70 z ≲ 0
    Yang, Qian et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    37
  • Determinación de orientaciones de ciudades romanas por medio de la varatio / Orientation layout of Roman towns by using the varatio
    En el presente artículo se aborda la tan debatida cuestión de las orientaciones de ciudades romanas combinando dos procedimientos: un análisis estadístico de las orientaciones de una muestra significativa de ciudades romanas en la península ibérica, y los resultados de una investigación basada en la experimentación y reconstrucción de instrumental
    Orfila Pons, M. et al.

    Fecha de publicación:

    9
    2020
  • Cosmic Amorphous Dust Model as the Origin of Anomalous Microwave Emission
    We have shown that the thermal emission of the amorphous dust composed of amorphous silicate dust (a-Si) and amorphous carbon dust (a-C) provides an excellent fit both to the observed intensity and the polarization spectra of molecular clouds. The anomalous microwave emission (AME) originates from the resonance transition of the two-level systems
    Nashimoto, Masashi et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    13
  • Constraining the oblateness of transiting planets with photometry and spectroscopy
    Rapid planetary rotation can cause the equilibrium shape of a planet to be oblate. While planetary oblateness has mostly been probed by examining the subtle ingress and egress features in photometric transit light curves, we investigate the effect of oblateness on the spectroscopic Rossiter-McLaughlin (RM) signals. We found that a giant planet
    Akinsanmi, B. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    5
  • Completing the 3CR Chandra Snapshot Survey: Extragalactic Radio Sources at High Redshift
    We present the analysis of nine radio sources belonging to the Third Cambridge Revised catalog (3CR) observed with Chandra during Cycle 20 in the redshift range between 1.5 and 2.5. This study completes the 3CR Chandra Snapshot Survey thus guaranteeing the X-ray coverage of all 3CR sources identified to date. This sample lists two compact steep
    Jimenez-Gallardo, A. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    17