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/

  • Observational evidence of different formation mechanisms of Solar System-type architectures across spectral types

    Despite being the most abundant classes of known exoplanets, super-Earths and mini-Neptunes are absent in our Solar System, and the exact reason for this is still unknown. Some models suggest that cold-Jupiters play a major role in the formation of inner low-mass planets. This could explain the current architecture of our Solar System, and the

    Pinamonti, Matteo et al.

    Advertised on:

    4
    2024
    Citations
    0
  • Performance and first measurements of the MAGIC stellar intensity interferometer

    In recent years, a new generation of optical intensity interferometers has emerged, leveraging the existing infrastructure of Imaging Atmospheric Cherenkov Telescopes (IACTs). The MAGIC telescopes host the MAGIC-SII system (Stellar Intensity Interferometer), implemented to investigate the feasibility and potential of this technique on IACTs. After

    Abe, S. et al.

    Advertised on:

    4
    2024
    Citations
    1
  • Planets observed with CHEOPS. Two super-Earths orbiting the red dwarf star TOI-776

    Context. M-dwarf stars are the most common of potential exoplanet host stars in the Galaxy. It is therefore very important to understand planetary systems orbiting such stars and to determine the physical parameters of such planets with high precision. Also with the launch of the James Webb Space Telescope (JWST) the observation of atmospheric

    Fridlund, M. et al.

    Advertised on:

    4
    2024
    Citations
    0
  • Revisiting the warm sub-Saturn TOI-1710b. The impact of stellar activity on the mass measurement

    The Transiting Exoplanet Survey Satellite (TESS) provides a continuous suite of new planet candidates that need confirmation and precise mass determination from ground-based observatories. This is the case for the G-type star TOI-1710, which is known to host a transiting sub-Saturn planet (M p = 28.3 ± 4.7 M ⊕) in a long-period orbit (P = 24.28

    Orell-Miquel, J. et al.

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    4
    2024
    Citations
    0
  • Soft-state optical spectroscopy of the black hole MAXI J1305-704

    The X-ray dipper MAXI J1305-704 is a dynamically confirmed black hole (BH) X-ray binary discovered a decade ago. While its only outburst has been studied in detail in X-rays, follow-up at other wavelengths has been scarce. We report here the results from an optical spectroscopy campaign across the outburst of MAXI J1305-704. We analysed two epochs

    Miceli, C. et al.

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    4
    2024
    Citations
    0
  • Teegarden's Star revisited. A nearby planetary system with at least three planets

    The two known planets in the planetary system of Teegarden's Star are among the most Earth-like exoplanets currently known. Revisiting this nearby planetary system with two planets in the habitable zone aims at a more complete census of planets around very low-mass stars. A significant number of new radial velocity measurements from CARMENES

    Dreizler, S. et al.

    Advertised on:

    4
    2024
    Citations
    0