Publicaciones en colaboración con investigadores/as de Ames Research Center (23)

2014

  1. The PLATO 2.0 mission

    Experimental Astronomy, Vol. 38, Núm. 1-2, pp. 249-330

2012

  1. Fundamental properties of five Kepler stars using global asteroseismic quantities and ground-based observations

    Astronomy and Astrophysics, Vol. 537

  2. Kepler observations of the high-amplitude δScuti star V2367Cyg

    Monthly Notices of the Royal Astronomical Society, Vol. 419, Núm. 4, pp. 3028-3038

2011

  1. Atmospheric parameters and pulsational properties for a sample of δSct, γDor and hybrid Kepler targets

    Monthly Notices of the Royal Astronomical Society, Vol. 411, Núm. 2, pp. 1167-1176

  2. Kepler observations of the variability in B-type stars

    Monthly Notices of the Royal Astronomical Society, Vol. 413, Núm. 4, pp. 2403-2420

  3. Regularities in frequency spacings of δ Scuti stars: The Kepler star KIC9700322

    Monthly Notices of the Royal Astronomical Society, Vol. 414, Núm. 2, pp. 1721-1731

  4. The Kepler characterization of the variability among A-and F-type stars: I. General overview

    Astronomy and Astrophysics, Vol. 534

2010

  1. A precise asteroseismic age and radius for the evolved sun-like star KIC 11026764

    Astrophysical Journal, Vol. 723, Núm. 2, pp. 1583-1598

  2. Detection of solar-like oscillations from kepler photometry of the open cluster NGC 6819

    Astrophysical Journal Letters, Vol. 713, Núm. 2 PART 2

  3. Hybrid γdORADUS-δScuti Pulsators: New insights into the physics of the oscillations from kepler observations

    Astrophysical Journal Letters, Vol. 713, Núm. 2 PART 2

  4. Kepler asteroseismology program: Introduction and first results

    Publications of the Astronomical Society of the Pacific, Vol. 122, Núm. 888, pp. 131-143

  5. Kepler observations: Light shed on the hybrid γ Doradus - δ Scuti pulsation phenomenon

    Astronomische Nachrichten, Vol. 331, Núm. 9-10, pp. 989-992

  6. The asteroseismic potential of kepler: First results for solar-type stars

    Astrophysical Journal Letters, Vol. 713, Núm. 2 PART 2