Dynamical modelling of giant radio quasars in the HETDEX Spring Field

arXiv:2607.12964 · astro-ph.GA · Submitted 2026-07-14 · Read on arXiv

T. M. O. Franzen, J. Machalski, M. Jamrozy, R. Morganti, D. A. Green, Y. C. Perrott, T. W. Shimwell

ASTRON, the Netherlands Institute for Radio Astronomy, Dwingeloo, The Netherlands · Astronomical Observatory, Jagiellonian University, Krakow, Poland · Astronomical Observatory, Jagiellonian University, Krakow, Poland · Kapteyn Astronomical Institute, University of Groningen, Groningen, The Netherlands · Astrophysics Group, Cavendish Laboratory, Cambridge, UK · School of Chemical and Physical Sciences, Victoria University of Wellington, Wellington, New Zealand · Leiden Observatory, Leiden University, Leiden, The Netherlands

astro-ph.GA

Submitted: 2026-07-14

Comments: Accepted for publication in MNRAS

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 47× in this paper · explained in 2 episodes
• AGN — 10× in this paper · explained in 1 episode
• Anti-correlation — 4× in this paper · explained in 3 episodes
• Calibration — 4× in this paper · explained in 7 episodes
• Large Array — 2× in this paper
• Accretion Flows — 1× in this paper · explained in 1 episode
• Canadian Initiative for Radio Astronomy Data Analysis — 1× in this paper
• Degeneracy — 1× in this paper · explained in 3 episodes
• Frequency Dependence — 1× in this paper · explained in 2 episodes
• Inverse Problem — 1× in this paper · explained in 2 episodes
• NRAO Very Large Array — 1× in this paper
• Owens Valley Radio Observatory — 1× in this paper

Related papers

• Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
• Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
• Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
• Deriving volume density profiles of filaments from observed surface densities
• Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
• MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies