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/

  • A self-consistent direct method for chemical abundances in high-z galaxies with JWST
    The unprecedented rest-frame UV and optical coverage provided by James Webb Space Telescope (JWST) enables simultaneous constraints on the electron density ( $n_{\rm e}$) and temperature ( $T_{\rm e}$) of ionized gas in galaxies at $z\,\gt\,5$. We present a self-consistent direct method based on multiple O III] ( $\lambda \lambda$1661, 1666) and [O
    Arellano-Córdova, K. Z. et al.

    Advertised on:

    4
    2026
    Citations
    0
  • A search for optical counterparts in quiescent black hole X-ray transients
    Dynamical mass measurements of compact stars in X-ray transients demand the detection of optical/near-infrared counterparts in quiescence. Out of the 73 black hole candidates in X-ray transients, optical and near-infrared quiescent counterparts have only been identified for 34 objects. We present ULTRACAM photometric observations of nine candidate
    Yanes-Rizo, I. V. et al.

    Advertised on:

    4
    2026
    Citations
    0
  • A high-resolution X-ray view of the ultra-fast outflow in MAXI J1810−222
    Context. The Galactic black hole candidate MAXI J1810−222 was recently reported to exhibit a notable absorption spectral feature at around 1 keV in low-resolution X-ray spectra from detectors resembling charge-coupled devices. The feature is typically correlated with the spectral state of the source being stronger in the soft states, as often
    Pinto, C. et al.

    Advertised on:

    4
    2026
    Citations
    0
  • A Ground-based Transit Observation of the Long-period Extremely Low-density Planet HIP 41378 f
    We present a ground-based transit detection of HIP 41378 f, a long-period (P = 542 days), extremely low-density (0.09 ± 0.02 g cm −3) giant exoplanet in a dynamically complex system. Using photometry from Tierras, TRAPPIST-North, and multiple Las Cumbres Observatory Global Telescope sites, we constrain the transit center time to T C,6 = 2460438.891
    García-Mejía, Juliana et al.

    Advertised on:

    4
    2026
    Citations
    1
  • A comparison of pendulum models for large-amplitude longitudinal prominence oscillations
    Large-amplitude prominence oscillations offer diagnostic information relevant to understanding the magnetic and plasma structure of solar prominences. Accurate prominence seismology requires the use of reliable models. The so-called pendulum model for large-amplitude longitudinal prominence oscillations has demonstrated robustness against
    Arregui, Iñigo

    Advertised on:

    4
    2026
    Citations
    0
  • 3I/ATLAS: In Search of the Witnesses to Its Voyage
    3I/ATLAS is the third interstellar object discovered to date, following 1I/'Oumuamua and 2I/Borisov. Its unusually high excess velocity and active cometary nature make it a key probe of the Galactic population of icy planetesimals. Understanding its origin requires its past trajectory through the Galaxy to be traced and the possible role of stellar
    Pérez-Couto, X. et al.

    Advertised on:

    4
    2026
    Citations
    7