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
    Measurement of Atmospheric Scintillation during a Period of Saharan Dust (Calima) at Observatorio del Teide, Iz̃ana, Tenerife, and the Impact on Photometric Exposure Times
    We present scintillation noise profiles captured at the Observatorio del Teide, Izaña, Tenerife, over a one-week period in 2017 September. Contemporaneous data from the Birmingham Solar Oscillations Network (BiSON) and the Stellar Activity (STELLA) robotic telescopes provides estimates of daily atmospheric extinction allowing the scintillation
    Hale, S. J. et al.

    Fecha de publicación:

    3
    2020
    Bibcode
    2020PASP..132c4501H
    Número de citas
    5
  • Con árbitro
    MEGARA-GTC stellar spectral library: I
    MEGARA (Multi Espectrógrafo en GTC de Alta Resolución para Astronomía) is an optical (3650-9750 Å), fibre-fed, medium-high spectral resolution (R = 6000, 12 000 and 20 000) instrument for the Gran Telescopio CANARIAS (GTC) 10.4-m telescope, commissioned in the summer of 2017, and currently in operation. The scientific exploitation of MEGARA
    García-Vargas, M. L. et al.

    Fecha de publicación:

    3
    2020
    Bibcode
    2020MNRAS.493..871G
    Número de citas
    10
  • Con árbitro
    Monitoring of the radio galaxy M 87 during a low-emission state from 2012 to 2015 with MAGIC
    M 87 is one of the closest (z = 0.004 36) extragalactic sources emitting at very high energies (VHE, E > 100 GeV). The aim of this work is to locate the region of the VHE gamma-ray emission and to describe the observed broad-band spectral energy distribution (SED) during the low VHE gamma-ray state. The data from M 87 collected between 2012 and
    MAGIC Collaboration et al.

    Fecha de publicación:

    3
    2020
    Bibcode
    2020MNRAS.492.5354M
    Número de citas
    38
  • Con árbitro
    Multiplicity of the red supergiant population in the young massive cluster NGC 330
    Context. The multiplicity properties of massive stars are one of the important outstanding issues in stellar evolution. Quantifying the binary statistics of all evolutionary phases is essential to paint a complete picture of how and when massive stars interact with their companions, and to determine the consequences of these interactions. Aims: We
    Patrick, L. R. et al.

    Fecha de publicación:

    3
    2020
    Bibcode
    2020A&A...635A..29P
    Número de citas
    16
  • Con árbitro
    Multiwavelength behaviour of the blazar 3C 279: decade-long study from γ-ray to radio
    We report the results of decade-long (2008-2018) γ-ray to 1 GHz radio monitoring of the blazar 3C 279, including GASP/WEBT, Fermi and Swift data, as well as polarimetric and spectroscopic data. The X-ray and γ-ray light curves correlate well, with no delay ≳ 3 h, implying general cospatiality of the emission regions. The γ-ray-optical flux-flux
    Larionov, V. M. et al.

    Fecha de publicación:

    3
    2020
    Bibcode
    2020MNRAS.492.3829L
    Número de citas
    41
  • Con árbitro
    New Hard-TeV Extreme Blazars Detected with the MAGIC Telescopes
    Extreme high-frequency-peaked BL Lac objects (EHBLs) are blazars that exhibit extremely energetic synchrotron emission. They also feature nonthermal gamma-ray emission whose peak lies in the very high-energy (VHE, E > 100 GeV) range, and in some sources exceeds 1 TeV: this is the case for hard-TeV EHBLs such as 1ES 0229+200. With the aim of
    Acciari, V. A. et al.

    Fecha de publicación:

    3
    2020
    Bibcode
    2020ApJS..247...16A
    Número de citas
    47