Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • LOFAR MSSS: detection of a low-frequency radio transient in 400 h of monitoring of the North Celestial Pole
    We present the results of a four-month campaign searching for low-frequency radio transients near the North Celestial Pole with the Low-Frequency Array (LOFAR), as part of the Multifrequency Snapshot Sky Survey (MSSS). The data were recorded between 2011 December and 2012 April and comprised 2149 11-min snapshots, each covering 175 deg2. We have
    Stewart, A. J. et al.

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    3
    2016
    Citations
    65
  • Inferring planetary obliquity using rotational and orbital photometry
    The obliquity of a terrestrial planet is an important clue about its formation and critical to its climate. Previous studies using simulated photometry of Earth show that continuous observations over most of a planet's orbit can be inverted to infer obliquity. However, few studies of more general planets with arbitrary albedo markings have been
    Schwartz, J. C. et al.

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    3
    2016
    Citations
    42
  • Heating of the Partially Ionized Solar Chromosphere by Waves in Magnetic Structures
    In this paper, we show a “proof of concept” of the heating mechanism of the solar chromosphere due to wave dissipation caused by the effects of partial ionization. Numerical modeling of non-linear wave propagation in a magnetic flux tube, embedded in the solar atmosphere, is performed by solving a system of single-fluid quasi-MHD equations, which
    Shelyag, S. et al.

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    3
    2016
    Citations
    58
  • Erratum: “Results of a Search for γ Dor and δ Sct Stars with the Kepler Spacecraft” (2015, AJ, 149, 68)
    Not Available
    Jackiewicz, J. et al.

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    3
    2016
    Citations
    1
  • Early-type dwarf galaxies with multicomponent stellar structure: Are they remnants of disc galaxies strongly transformed by their environment?
    Context. The surface brightness distribution of ~30-40% of the early-type dwarf galaxies with - 18 ≤ MB ≤ -15 in the Virgo and the Coma clusters is fitted by models that include two structural components (Sérsic + exponential) as for bright disc galaxies. Aims: The goal of the present study is to determine whether early-type dwarf galaxies with a
    Aguerri, J. A. L.

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    3
    2016
    Citations
    11