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/

  • TOI-1268b: The youngest hot Saturn-mass transiting exoplanet
    We report the discovery of TOI-1268b, a transiting Saturn-mass planet from the TESS space mission. With an age of less than 1 Gyr, derived from various age indicators, TOI-1268b is the youngest Saturn-mass planet known to date; it contributes to the small sample of well-characterised young planets. It has an orbital period of P = 8.1577080 ± 0
    Šubjak, J. et al.

    Advertised on:

    6
    2022
    Citations
    10
  • TOI-178: a window into the formation and evolution of planetary systems
    Laplacian resonant chains — where astronomical bodies are in mean motion resonance with two or more other bodies — are rare phenomena observed in systems such as the TRAPPIST-1 exoplanets and the Galilean moons of Jupiter. Laplacian chains are an important tool to study the history of planetary systems occupying this configuration, as the fragility
    Hooton, Matthew J. et al.

    Advertised on:

    6
    2022
    Citations
    0
  • TOI-2136b: a sub-Neptune planet around a nearby M3 dwarf
    Small planets with a radius between 1-4 Earth radii are extremely common in the Milky Way but their planetary formation and evolution are not revealed completely. NASA's Kepler space telescope revealed that this population has a bimodal distribution to be consistent with the transition from rocky to non-rocky planets predicted by photoevaporation
    Kawauchi, Kiyoe et al.

    Advertised on:

    6
    2022
    Citations
    0
  • Transit Timing Variations for AU Microscopii b & c
    We explore the transit timing variations (TTVs) of the young (22 Myr) nearby AU Mic planetary system. For AU Mic b, we introduce three Spitzer (4.5 μm) transits, five TESS transits, 11 LCO transits, one PEST transit, one Brierfield transit, and two transit timing measurements from Rossiter-McLaughlin observations; for AU Mic c, we introduce three
    Wittrock, Justin M. et al.

    Advertised on:

    6
    2022
    Citations
    0
  • V1298 Tau - Rapid contraction of giant planets?
    Current theories predict that very young giant planets have large radii and very low densities before they slowly contract to reach their final size after several hundred million years. Open stellar clusters and young moving groups of stars offer a unique opportunity to study exoplanets at their infant stages because of the well-constrained ages
    Suárez Mascareño, Alejandro

    Advertised on:

    6
    2022
    Citations
    0
  • The Origin of Weakened Magnetic Braking in Old Solar Analogs
    The rotation rates of main-sequence stars slow over time as they gradually lose angular momentum to their magnetized stellar winds. The rate of angular momentum loss depends on the strength and morphology of the magnetic field, the mass-loss rate, and the stellar rotation period, mass, and radius. Previous observations suggested a shift in magnetic
    Metcalfe, Travis S. et al.

    Advertised on:

    7
    2022
    Citations
    27