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/

  • Proxima Centauri b is not a transiting exoplanet
    We report Spitzer Space Telescope observations during predicted transits of the exoplanet Proxima Centauri b. As the nearest terrestrial habitable-zone planet we will ever discover, any potential transit of Proxima b would place strong constraints on its radius, bulk density, and atmosphere. Subsequent transmission spectroscopy and secondary
    Jenkins, James S. et al.

    Advertised on:

    7
    2019
    Citations
    24
  • Properties of the Umbral Filament Observed in Active Region NOAA 12529
    Recent observations of the solar photosphere revealed the presence of elongated filamentary bright structures inside sunspot umbrae, called umbral filaments (UFs). These features differ in morphology, magnetic configuration, and evolution from light bridges (LBs) that are usually observed to intrude in sunspots. To characterize a UF observed in the
    Guglielmino, Salvo L. et al.

    Advertised on:

    7
    2019
    Citations
    16
  • Polyvinyl alcohol cryogel phantoms of biological tissues for wideband operation at microwave frequencies
    The aim of this work is to provide a methodology to model the dielectric properties of human tissues based on phantoms prepared with an aqueous solution, in a semi-solid form, by using off-the-shelf components. Polyvinyl alcohol cryogel (PVA-C) has been employed as a novel gelling agent in the fabrication of phantoms for microwave applications in a
    N. Arteaga-Marrero et al.

    Advertised on:

    7
    2019
  • Origin of the chromospheric three-minute oscillations in sunspot umbrae
    Context. Sunspot umbrae show a change in the dominant period of their oscillations from five minutes (3.3 mHz) in the photosphere to three minutes (5.5 mHz) in the chromosphere. Aims: In this paper, we explore the two most popular models proposed to explain the three-minute oscillations: the chromospheric acoustic resonator and the propagation of
    Felipe, T.

    Advertised on:

    7
    2019
    Citations
    22
  • Optical/NIR stellar absorption and emission-line indices from luminous infrared galaxies
    We analyse a set of optical-to-near-infrared long-slit nuclear spectra of 16 infrared-luminous spiral galaxies. All of the studied sources present H2 emission, which reflects the star-forming nature of our sample, and they clearly display H I emission lines in the optical. Their continua contain many strong stellar absorption lines, with the most
    Riffel, R. et al.

    Advertised on:

    7
    2019
    Citations
    30
  • Optical and X-ray correlations during the 2015 outburst of the black hole V404 Cyg
    We present a serendipitous multiwavelength campaign of optical photometry simultaneous with Integral X-ray monitoring of the 2015 outburst of the black hole V404 Cyg. Large-amplitude optical variability is generally correlated with X-rays, with lags of order a minute or less compatible with binary light travel time-scales or jet ejections. Rapid
    Hynes, R. I. et al.

    Advertised on:

    7
    2019
    Citations
    11