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/

  • Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies
    The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, the short gamma-ray burst GRB 170817A, heralded the birth of multimessenger astronomy. The detection of TeV emission from GRBs motivates follow-up observations with the
    Abe, S. et al.

    Advertised on:

    6
    2026
    Citations
    1
  • Beyond single tracers: Convolutional neural network-based inference of galaxy mass profiles from combined gas and stellar kinematics
    Aims. We investigated whether combining gas and stellar kinematic maps provides measurable advantages in recovering galaxy mass profiles compared to using single-component maps alone. We used deep learning models to leverage this joint information. Methods. We developed a probabilistic convolutional neural network (CNN) framework trained and tested
    Expósito-Márquez, J. et al.

    Advertised on:

    6
    2026
    Citations
    0
  • Astrophysical parameters of LS 437 and the nature of X0726─260
    Context. Be/X-ray binaries, the most common class of high-mass X-ray binaries, are characterised by OBe companions, but they display a rich variety of X-ray behaviours. One of the most atypical systems is X0726−260, which also has the earliest optical counterpart among the whole Milky Way and Magellanic Cloud sample. Aims. We intend to improve the
    Negueruela, I. et al.

    Advertised on:

    6
    2026
    Citations
    0
  • Ariel stellar characterisation: IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample
    Context. The characterisation of exoplanetary systems depends on the accurate determination of host star parameters. The Ariel mission will probe the atmospheres of a statistically significant sample of exoplanets, and so requires a precise characterisation of the stellar properties well before its launch in 2031. The homogeneous determination of
    Ramler, H. et al.

    Advertised on:

    6
    2026
    Citations
    1
  • Aql X-1 from dawn 'til dusk: the early rise, fast state transition, and decay of its 2024 outburst
    Transient low-mass X-ray binaries (LMXBs) are usually first detected by all-sky X-ray monitors when they enter new outbursts. These detections typically occur at X-ray luminosities above ∼10 36 erg/s. Observations of these sources during the early rise of the outbursts have therefore been very limited so far. However, the launch of the Einstein
    Marino, A. et al.

    Advertised on:

    6
    2026
    Citations
    3
  • Ancient 'ghost' planetary nebulae discovered with amateur telescopes
    As planetary nebulae evolve, they fade and dissipate into the surrounding interstellar medium, which makes them harder to detect. Modern, advanced amateur equipment can help to uncover this hidden population of ancient 'ghost' planetary nebulae. Via careful processing of long-integration, narrow-band imagery with modest aperture telescopes at a
    Manuel, J. A. et al.

    Advertised on:

    6
    2026
    Citations
    0