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/

  • Are early-type galaxies quenched by present-day environment?: A study of dwarfs in the Fornax Cluster
    Galaxies undergo numerous transformative processes throughout their lifetimes that ultimately lead to the expulsion of gas and the cessation of star-forming activity. This phenomenon is commonly known as quenching, and in this study, we delve into the possibility that this process is caused by the environmental processes associated with the
    Romero-Gómez, J. et al.

    Advertised on:

    9
    2024
    Citations
    0
  • Characterisation of the warm-Jupiter TOI-1130 system with CHEOPS and a photo-dynamical approach
    Context. Among the thousands of exoplanets discovered to date, approximately a few hundred gas giants on short-period orbits are classified as 'lonely' and only a few are in a multi-planet system with a smaller companion on a close orbit. The processes that formed multi-planet systems hosting gas giants on close orbits are poorly understood, and
    Borsato, L. et al.

    Advertised on:

    9
    2024
    Citations
    0
  • Deriving the star formation histories of galaxies from spectra with simulation-based inference
    High-resolution galaxy spectra encode information about the stellar populations within galaxies. The properties of the stars, such as their ages, masses, and metallicities, provide insights into the underlying physical processes that drive the growth and transformation of galaxies over cosmic time. We explore a simulation-based inference (SBI)
    Iglesias-Navarro, Patricia et al.

    Advertised on:

    9
    2024
    Citations
    0
  • ESPRESSO reveals blueshifted neutral iron emission lines on the dayside of WASP-76 b
    Context. Ultra hot Jupiters (gas giants with T eq > 2000 K) are intriguing exoplanets due to the extreme physics and chemistry present in their atmospheres. Their torrid daysides can be characterised using ground-based high-resolution emission spectroscopy. Aims. We search for signatures of neutral and singly ionised iron (Fe I and Fe II
    Costa Silva, A. R. et al.

    Advertised on:

    9
    2024
    Citations
    0
  • From gas to stars: MUSEings on the internal evolution of IC 1613
    Context. The kinematics and chemical composition of stellar populations of different ages provide crucial information on the evolution of the various components of a galaxy. Aim. Our aim is to determine the kinematics of individual stars as a function of age in IC 1613, a star-forming, gas-rich, and isolated dwarf galaxy of the Local Group (LG)
    Taibi, S. et al.

    Advertised on:

    9
    2024
    Citations
    0
  • The atmospheric composition of the ultra-hot Jupiter WASP-178 b observed with ESPRESSO
    Context. Ultra-hot Jupiters (UHJ) have emerged as ideal testbeds for new techniques for studying exoplanet atmospheres. Only a limited number of them are currently well studied, however. Aims. We search for atmospheric constituents for the UHJ WASP-178 b with two ESPRESSO transits. Additionally, we show parallel photometry that we used to obtain
    Damasceno, Y. C. et al.

    Advertised on:

    9
    2024
    Citations
    0