• Publication
    Accelerating 3D non-LTE synthesis with graph neural networks
    Context. Spectropolarimetric interpretation of chromospheric lines requires solving the radiative transfer problem under non-local thermodynamic equilibrium...
  • Publication
    Accelerating Multiframe Blind Deconvolution via Deep Learning
    Ground-based solar-image restoration is a computationally expensive procedure that involves nonlinear optimization techniques. The presence of atmospheric...
  • Publication
    Accelerating Non-LTE Synthesis and Inversions with Graph Networks
    The computational cost of fast non-LTE synthesis is one of the challenges that limits the development of 2D and 3D inversion codes. It also makes the...
  • Publication
    Accreting magnetars: a new type of high-mass X-ray binaries?
    The discovery of very slow pulsations (Pspin =5560 s) has solved the long-standing question of the nature of the compact object in the high-mass X-ray binary 4U...
  • Publication
    Accretion and Outflow in the Proplyd-like Objects Near Cygnus OB2
    Cygnus OB2 is the most massive association within 2 kpc from the Sun, hosting hundreds of massive stars, thousands of young low mass members, and some sights of...
  • Publication
    Accretion and outflow in V404 Cyg
    We study the optical evolution of the 2015 outburst in V404 Cyg, with emphasis on the peculiar nebular phase and subsequent decay to quiescence. From the decay...
  • Publication
    Accretion and UV Variability in BP Tauri
    BP Tau is one of the few classical T Tauri stars for which the presence of a hot spot in the surface has been reported without ambiguity. The most likely source...
  • Publication
    Accretion disc winds imprint distinct signatures in the optical variability spectrum of black hole transients
    Quantifying the variability, measured as the root mean square (rms), of accreting systems as a function of energy is a powerful tool for constraining the...
  • Publication
    Accretion Disc Winds in X-ray Binaries
    Despite early theoretical expectations that large-scale, massive outflows would be triggered by accretion onto black holes and neutron stars, their presence was...