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/

  • Implications of the Intriguing Constant Inner Mass Surface Density Observed in Dark Matter Halos
    It has long been known that the observed mass surface density of cored dark matter (DM) halos is approximately constant, independently of the galaxy mass (i.e., ρ c r c ≃ constant, with ρ c and r c being the central volume density and the radius of the core, respectively). Here, we review the evidence supporting this empirical fact as well as its
    Sánchez Almeida, Jorge

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    1
    2025
    Citations
    0
  • Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles
    Complementary to high-energy experimental efforts, indirect astrophysical searches of particles beyond the standard model have long been pursued. The present article follows the latter approach and considers, for the first time, the self-consistent treatment of the energy losses from dark flavoured particles produced in the decay of hyperons during
    Fischer, Tobias et al.

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    1
    2025
    Citations
    1
  • High-resolution observational analysis of flare ribbon fine structures
    Context. Since the mechanism of energy release from solar flares is still not fully understood, the study of fine-scale features developing during flares becomes important for progressing towards a consistent picture of the essential physical mechanisms. Aims. Solar flares release most of their luminous energy in the chromosphere. These luminous
    Thoen Faber, Jonas et al.

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    1
    2025
    Citations
    0
  • HD 119130 b Is Not an "Ultradense" Sub-Neptune
    We present a revised mass measurement for HD 119130 b (aka K2-292 b), a transiting planet (P = 17 days, R p = R ⊕) orbiting a chromospherically inactive G dwarf, previously thought to be one of the densest sub-Neptunes known. Our follow-up Doppler observations with HARPS, HARPS-N, and HIRES reveal that HD 119130 b is, in fact, nearly one-third as
    Akana Murphy, Joseph M. et al.

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    1
    2025
    Citations
    0
  • HD 119130 b Is Not an "Ultradense" Sub-Neptune
    We present a revised mass measurement for HD 119130 b (aka K2-292 b), a transiting planet (P = 17 days, R p = 2.63 ‑ 0.10 + 0.11 R ⊕) orbiting a chromospherically inactive G dwarf, previously thought to be one of the densest sub-Neptunes known. Our follow-up Doppler observations with HARPS, HARPS-N, and HIRES reveal that HD 119130 b is, in fact
    Akana Murphy, Joseph M. et al.

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    1
    2025
    Citations
    1
  • Fiducial-cosmology-dependent systematics for the DESI 2024 BAO analysis
    When measuring the Baryon Acoustic Oscillations (BAO) scale from galaxy surveys, one typically assumes a fiducial cosmology when converting redshift measurements into comoving distances and also when defining input parameters for the reconstruction algorithm. A parameterised template for the model to be fitted is also created based on a (possibly
    Pérez-Fernández, A. et al.

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    1
    2025
    Citations
    16