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/

  • Multiband, Multiepoch Photometry of the Spot-crossing System TOI-3884: Refined System Geometry and Spot Properties
    Spot-crossing transits offer a unique opportunity to probe spot properties such as temperature, size, and surface distribution. TOI-3884 is a rare system in which spot-crossing features are persistently observed during every transit. This is due to its unusual configuration: a nearly polar-orbit super-Neptune transits a pole-on mid-M dwarf
    Mori, Mayuko et al.

    Advertised on:

    10
    2025
    Citations
    3
  • Measuring Rotation Periods from TESS in PLATO LOPS2 Fields
    NASA's Transiting Exoplanet Survey Satellite (TESS) has been conducting high-precision photometric observations for over seven years, covering more than 95% of the sky. By the end of Cycle 8, over 90% of this coverage will include observations from multiple sectors. The upcoming ESA PLAnetary Transits and Oscillations of Stars (PLATO; Rauer et al
    Palakkatharappil, Dinil Bose et al.

    Advertised on:

    10
    2025
    Citations
    0
  • joshspeagle/dynesty: v3.0.0
    This is major release with several infrastructural changes that will make future development of dynesty easier, as well as significant speedups. The release also deprecated some rarely used options. Major refactor of the code that makes it easier to add new samplers. Major speedup of the uniform sampler when sampling in parallel You can now provide
    Koposov, Sergey et al.

    Advertised on:

    10
    2025
    Citations
    2
  • Is turbulent convection the only exciting mechanism of acoustic modes in solar-like oscillators?
    The solar convective envelope generates, by dynamo effect, a surface magnetic field whose strength evolves on an 11-year cycle, with a change in polarity at the end of each cycle. A similar magnetic variability exists in other solar-type stars, influencing their dynamics. Furthermore, solar-like oscillators experience acoustic modes whose
    Panetier, Eva et al.

    Advertised on:

    10
    2025
    Citations
    0
  • Investigating Phosphorus Abundances in a Sample of APOGEE-2 Bulge Globular Clusters
    Phosphorus-enhanced (P-rich; [P/Fe] ≳ +0.8) giants have been found among mildly metal-poor field stars, but in only one star in a globular cluster (GC), M4 (NGC 6121). Also, in a sample of bulge spheroid stars, some of them showed a moderate P enhancement in the range +0.5 < [P/Fe] < +1.0. In this paper we derive the P abundance of moderately metal
    Barbuy, Beatriz et al.

    Advertised on:

    10
    2025
    Citations
    0
  • Identification of Nonlinear Damping of Transverse Loop Oscillations by KHI-induced Turbulence
    Kink oscillations in coronal loops have been extensively studied for their potential contributions to coronal heating and their role in plasma diagnostics through coronal seismology. A key focus is the strong damping of large-amplitude kink oscillations, which observational evidence suggests is nonlinear. However, directly identifying the
    Zhong, Sihui et al.

    Advertised on:

    10
    2025
    Citations
    0