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/

  • Using gas kinematics to measure resonant structures in disc galaxies: the interaction of M51 with NGC 5195
    Interstellar gas offers advantages when quantifying the structure of the resonances in disc galaxies. The gas is concentrated close to the disc mid-plane, making it easier to determine its in-plane velocity components, and it offers sharp emission lines for good velocity resolution. These properties are shared by atomic, molecular, and ionized gas
    Beckman, John et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Using autoencoders and deep transfer learning to determine the stellar parameters of 286 CARMENES M dwarfs
    Context. Deep learning (DL) techniques are a promising approach among the set of methods used in the ever-challenging determination of stellar parameters in M dwarfs. In this context, transfer learning could play an important role in mitigating uncertainties in the results due to the synthetic gap (i.e. difference in feature distributions between
    Mas-Buitrago, P. et al.

    Advertised on:

    7
    2024
    Citations
    6
  • Use of a finite state machine approach for sequence control in the GREGOR infrared spectrograph (GRIS)
    Due to the complexity of scientific instruments, such as spectropolarimeters, managing instrument sequences can be challenging. To address this problem, a Finite-State Machine (FSM) approach has been used to manage solar observation sequences in the GREGOR Infrared Spectrograph (GRIS). FSMs provide a structured and visual representation of control
    Matta-Gómez, A. et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Unveiling the central kpc of Type I AGN host galaxies in seeing-limited IFS data
    The evolution of galaxies appears linked to the growth of supermassive black holes (SMBH), as evidenced by empirical scale relations between hosts' large-scale properties and the mass of their central black holes. This co-evolutionary scenario suggests that all galaxies experience nuclear activity — active phases during which the black hole
    García Lorenzo, Begoña et al.

    Advertised on:

    7
    2024
    Citations
    0
  • Unveiling the (in)consistencies among the galaxy stellar mass function, star formation histories, satellite abundances, and intracluster light from a semi-empirical perspective
    In a hierarchical, dark matter-dominated Universe, stellar mass functions (SMFs), galaxy merger rates, star formation histories (SFHs), satellite abundances, and intracluster light (ICL), should all be intimately connected observables. However, the systematics affecting observations still prevent universal and uniform measurements of, for example
    Fu, Hao et al.

    Advertised on:

    7
    2024
    Citations
    8
  • Unveiling galaxy protoclusters in the era of Euclid
    How large-scale structures formed in the early universe is a key cosmological question with few answers from empirical evidence. Unveiling galaxy clusters and their high-z progenitors (i.e., protoclusters) is essential to picture galaxy evolution drawn by the hierarchical formation scenario. However, unveiling these early structures at high
    Ramos Chernenko, Nataliya et al.

    Advertised on:

    7
    2024
    Citations
    0