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/

  • INSPIRE: INvestigating Stellar Populations In RElics - IX. KiDS J0842 + 0059: the first fully confirmed relic beyond the local Universe
    Relics are massive, compact and quiescent galaxies that assembled the majority of their stars in the early Universe and lived untouched until today, completely missing any subsequent size growth caused by mergers and interactions. They provide the unique opportunity to put constraints on the first phase of mass assembly in the Universe with the
    Tortora, C. et al.

    Advertised on:

    7
    2025
    Citations
    0
  • Is the symbiotic recurrent nova T CrB late? Recent photometric evolution and comparison with past pre-outburst behaviour
    T CrB is a symbiotic recurrent nova that last erupted in 1946. Given its recurrence time-scale of approximately 80 yr, the next outburst is eagerly anticipated by the astronomical community. In this work, we analyse the optical light curves of T CrB, comparing recent photometric evolution with historical data to evaluate potential predictive
    Merc, Jaroslav et al.

    Advertised on:

    7
    2025
    Citations
    0
  • Improving galaxy cluster selection with the outskirt stellar mass of galaxies
    The number density and redshift evolution of optically selected galaxy clusters offer an independent measurement of the amplitude of matter fluctuations, S 8. However, recent results have shown that clusters chosen by the redMaPPer algorithm show richness-dependent biases that affect the weak lensing signals and number densities of clusters
    Kwiecien, Matthew et al.

    Advertised on:

    6
    2025
    Citations
    3
  • A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr
    Double white dwarf binaries are a leading explanation of the origin of type Ia supernovae, but no system exceeding the Chandrasekhar mass limit (1.4 M ⊙) has been found that will explode anywhere close to a Hubble time. Here we present the super-Chandrasekhar mass double white dwarf WDJ181058.67+311940.94 whose merger time (22.6 ± 1.0 Gyr) is of
    Munday, James et al.

    Advertised on:

    6
    2025
    Citations
    2
  • Analysis of optical spectroscopy and photometry of the type I X-ray bursting system UW CrB
    UW Coronae Borealis (UW CrB) is a low mass X-ray binary that shows both Type 1 X-ray and optical bursts, which typically last for 20 s. The system has a binary period of close to 2 hours and is thought to have a relatively high inclination due to the presence of an eclipse in the optical light curve. There is also evidence that an asymmetric disc
    Kennedy, Mark R. et al.

    Advertised on:

    6
    2025
    Citations
    0
  • Galaxy transformation across the cosmic web: Evolution of stellar colours and star formation rates in filaments
    Context. The aim of this work is to provide evidence of the imprints left by large-scale structure on galaxy properties by selecting extensive samples of galaxies from different environments, while matching their intrinsic and local environmental characteristics. Aims. We investigated the effects of the large-scale structure on the g ‑ r stellar
    Zarattini, S. et al.

    Advertised on:

    6
    2025
    Citations
    1