CHANG-ES XLII: Cosmic-Ray Electron Transport and the Spatially Resolved Radio-SFR Relation in Edge-on Galaxies

arXiv:2609.33211 · astro-ph.GA · Submitted 2026-09-27 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-27

Updated: 2026-09-27

Terminology

• Trace — 15× in this paper · explained in 2 episodes
• Calibration — 10× in this paper · explained in 7 episodes
• AGN — 7× in this paper · explained in 1 episode
• Frequency Dependence — 5× in this paper · explained in 2 episodes
• Consistency — 3× in this paper · explained in 3 episodes
• Core — 3× in this paper · explained in 2 episodes
• Robustness — 3× in this paper · explained in 5 episodes
• Baryonic Feedback — 1× in this paper · explained in 3 episodes
• Fidelity — 1× in this paper · explained in 2 episodes
• Jansky Very Large Array — 1× in this paper
• Orthogonal Distance Regression — 1× in this paper
• Star Formation Rate (SFR) — 1× in this paper · explained in 5 episodes

Sources

• Gemini: A Family of Highly Capable Multimodal Models
• Nearby galaxies in the LOFAR Two-metre Sky Survey IV. A fundamental plane of the radio-SFR relation

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