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/

  • Refereed
    Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu
    C-type asteroids 1 are considered to be primitive small Solar System bodies enriched in water and organics, providing clues to the origin and evolution of the Solar System and the building blocks of life. C-type asteroid 162173 Ryugu has been characterized by remote sensing 2-7 and on-asteroid measurements 8,9 with Hayabusa2 (ref. 10). However, the

    Advertised on:

    12
    2021
    Bibcode
    2021NatAs.tmp..255Y
  • Refereed
    Preliminary analysis of the Hayabusa2 samples returned from C-type asteroid Ryugu
    C-type asteroids 1 are considered to be primitive small Solar System bodies enriched in water and organics, providing clues to the origin and evolution of the Solar System and the building blocks of life. C-type asteroid 162173 Ryugu has been characterized by remote sensing 2-7 and on-asteroid measurements 8,9 with Hayabusa2 (ref. 10). However, the

    Advertised on:

    12
    2021
    Bibcode
    2021NatAs.tmp..265Y
  • Refereed
    Rapid contraction of giant planets orbiting the 20-million-year-old star V1298 Tau
    Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years 1,2. These theoretical expectations remain untested so far as the detection and characterization of very young planets is extremely

    Advertised on:

    12
    2021
    Bibcode
    2021NatAs.tmp..234S
  • Refereed
    Rapid contraction of giant planets orbiting the 20-million-year-old star V1298 Tau
    Current theories of planetary evolution predict that infant giant planets have large radii and very low densities before they slowly contract to reach their final size after about several hundred million years 1,2. These theoretical expectations remain untested so far as the detection and characterization of very young planets is extremely

    Advertised on:

    12
    2021
    Bibcode
    2021NatAs.tmp..252S
  • Refereed
    TOI-2285b: A 1.7 Earth-radius planet near the habitable zone around a nearby M dwarf
    We report the discovery of TOI-2285b, a sub-Neptune-sized planet transiting a nearby (42 pc) M dwarf with a period of 27.3 d. We identified the transit signal from the Transiting Exoplanet Survey Satellite photometric data, which we confirmed with ground-based photometric observations using the multiband imagers MuSCAT2 and MuSCAT3. Combining these

    Advertised on:

    12
    2021
    Bibcode
    2021PASJ..tmp..121F
  • Refereed
    Detections of solar-like oscillations in dwarfs and subgiants with Kepler DR25 short-cadence data
    During the survey phase of the Kepler mission, several thousand stars were observed in short cadence, allowing for the detection of solar-like oscillations in more than 500 main-sequence and subgiant stars. These detections showed the power of asteroseismology in determining fundamental stellar parameters. However, the Kepler Science Office
    Mathur, S. et al.

    Advertised on:

    1
    2022
    Bibcode
    2022A&A...657A..31M
    Citations
    18