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/

  • A Super-Earth and Sub-Neptune Transiting the Late-type M Dwarf LP 791-18
    Planets occur most frequently around cool dwarfs, but only a handful of specific examples are known to orbit the latest-type M stars. Using TESS photometry, we report the discovery of two planets transiting the low-mass star called LP 791-18 (identified by TESS as TOI 736). This star has spectral type M6V, effective temperature 2960 K, and radius 0
    Crossfield, Ian J. M. et al.

    Advertised on:

    9
    2019
    Citations
    52
  • A photometric and spectroscopic study of the multi-tailed asteroid (6478) Gault
    In this presentation, we describe several months of monitoring of Gault since January 2019 using various telescopes and instrumentation. The goal is to characterize and to model the asteroids and the tails to impose constraints on the physical properties of the ejected dust, and to shed light on the activity timeline and the causes for the ejection
    Jehin, Emmanuel et al.

    Advertised on:

    9
    2019
    Citations
    0
  • A giant exoplanet orbiting a very-low-mass star challenges planet formation models
    Surveys have shown that super-Earth and Neptune-mass exoplanets are more frequent than gas giants around low-mass stars, as predicted by the core accretion theory of planet formation. We report the discovery of a giant planet around the very-low-mass star GJ 3512, as determined by optical and near-infrared radial-velocity observations. The planet
    Morales, J. C. et al.

    Advertised on:

    9
    2019
    Citations
    111
  • A deeper look at the dust attenuation law of star-forming galaxies at high redshift
    A diverse range of dust attenuation laws is found in star-forming galaxies. In particular, Tress et al. (2018) studied the SHARDS survey to constrain the NUV bump strength (B) and the total-to-selective ratio (RV) of 1753 star-forming galaxies in the GOODS-N field at 1.5 z 3. We revisit here this sample to assess the implications and possible
    Tress, M. et al.

    Advertised on:

    9
    2019
    Citations
    9
  • TOI-216b and TOI-216 c: Two Warm, Large Exoplanets in or Slightly Wide of the 2:1 Orbital Resonance
    Warm, large exoplanets with 10–100 day orbital periods pose a major challenge to our understanding of how planetary systems form and evolve. Although high eccentricity tidal migration has been invoked to explain their proximity to their host stars, a handful reside in or near orbital resonance with nearby planets, suggesting a gentler history of in
    Dawson, Rebekah I. et al.

    Advertised on:

    8
    2019
    Citations
    23
  • The Starmus Festival - Our Primary Goal: Science Communication
    Starmus is a global festival of science communication and art that brings together the most brilliant minds on the planet. The festival is a gathering of top artists and scientists celebrated every two years. The aim of the project is to inspire and educate the next generation of explorers and regenerate the spirit of discovery. Starmus combines
    Israelian, Garik

    Advertised on:

    8
    2019
    Citations
    0