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/

  • Active optics strategy for the alignment and operation of the European Solar Telescope
    The European Solar Telescope (EST) is an on-axis 4.2-meter solar telescope, the largest solar telescope ever built in Europe. While operating, environmental effects, such as gravity, wind buffeting or thermal loads, will generate wavefront errors that require to be corrected. For this reason, the EST team is developing an active optics strategy to
    Belío-Asin, M. et al.

    Advertised on:

    8
    2022
    Citations
    0
  • A super-Earth orbiting near the inner edge of the habitable zone around the M4.5 dwarf Ross 508
    We report the near-infrared radial velocity (RV) discovery of a super-Earth planet on a 10.77 d orbit around the M4.5 dwarf Ross 508 (J mag = 9.1). Using precision RVs from the Subaru Telescope IRD (InfraRed Doppler) instrument, we derive a semi-amplitude of $3.92^{+0.60}_{-0.58}\:\mbox{m}\:{\mbox{s}^{-1}}$, corresponding to a planet with a minimum
    Harakawa, Hiroki et al.

    Advertised on:

    8
    2022
    Citations
    14
  • A stellar occultation by the transneptunian object (50000) Quaoar observed by CHEOPS
    Context. Stellar occultation is a powerful technique that allows the determination of some physical parameters of the occulting object. The result depends on the photometric accuracy, the temporal resolution, and the number of chords obtained. Space telescopes can achieve high photometric accuracy as they are not affected by atmospheric
    Morgado, B. E. et al.

    Advertised on:

    8
    2022
    Citations
    8
  • A slow bar in the lenticular barred galaxy NGC 4277
    Aims: We characterised the properties of the bar hosted in lenticular galaxy NGC 4277, which is located behind the Virgo cluster. Methods: We measured the bar length and strength from the surface photometry obtained from the broad-band imaging of the Sloan Digital Sky Survey and we derived the bar pattern speed from the stellar kinematics obtained
    Buttitta, C. et al.

    Advertised on:

    8
    2022
    Citations
    11
  • A pristine record of outer Solar System materials from asteroid Ryugu's returned sample
    Volatile and organic-rich C-type asteroids may have been one of the main sources of Earth's water. Our best insight into their chemistry is currently provided by carbonaceous chondritic meteorites, but the meteorite record is biased: only the strongest types survive atmospheric entry and are then modified by interaction with the terrestrial
    Ito, Motoo et al.

    Advertised on:

    8
    2022
    Citations
    69
  • A 2D Model for Coronal Bright Points: Association with Spicules, UV Bursts, Surges, and EUV Coronal Jets
    Coronal bright points (CBPs) are ubiquitous structures in the solar atmosphere composed of hot small-scale loops observed in extreme-ultraviolet (EUV) or X-rays in the quiet Sun and coronal holes. They are key elements to understanding the heating of the corona; nonetheless, basic questions regarding their heating mechanisms, the chromosphere
    Nóbrega-Siverio, D. et al.

    Advertised on:

    8
    2022
    Citations
    17