Journal: Astronomy and Astrophysics

  • Publication
    Feeding and feedback processes in the Spiderweb proto-intracluster medium
    Context. We present a detailed analysis of the thermal, diffuse emission of the proto-intracluster medium (proto-ICM) detected in the halo of the Spiderweb...
  • Publication
    Feeding and feedback processes in the Spiderweb proto-intracluster medium (Corrigendum)
  • Publication
    Feeding the spider with carbon. [CII] emission from the circumgalactic medium and active galactic nucleus
    We present the detection of [CII] 158 μm emission from the Spiderweb galaxy at z = 2.1612 using the Atacama Pathfinder EXperiment (APEX). The line profile...
  • Publication
    Field-aligned Evershed flows in the photosphere of a sunspot penumbra
    We determine the inclinations of the vector magnetic field and flow velocity in a sunspot penumbra by interpreting full Stokes profiles of three infrared lines...
  • Publication
    Field-level Lyman-α forest modeling in redshift space via augmented nonlocal Fluctuating Gunn-Peterson Approximation
    Context. Devising fast and accurate methods of predicting the Lyman-α forest at the field level, avoiding the computational burden of running large-volume...
  • Publication
    Finding galaxy clusters using Voronoi tessellations
    We present an objective and automated procedure for detecting clusters of galaxies in imaging galaxy surveys. Our Voronoi Galaxy Cluster Finder (VGCF) uses...
  • Publication
    Fine structure and dynamics in a light bridge inside a solar pore
    A photometric analysis of the sub-structure of a granular light bridge in a large solar pore is performed. The data consist of a 66 min time series of white...
  • Publication
    Fine structure in the Sigma Orionis cluster revealed by Gaia DR3
    Context. Sigma Orionis is an open cluster in the nearest giant star formation site - Orion. Its youth (3−5 Myr), low reddening, and relative vicinity make it an...
  • Publication
    FIR colours and SEDs of nearby galaxies observed with Herschel
    We present infrared colours (in the 25-500 μm spectral range) and UV to radio continuum spectral energy distributions of a sample of 51 nearby galaxies observed...