Abstract
An understanding of the relationship between radio-loud active galaxies and their large-scale environments is essential for realistic modelling of radio-galaxy evolution and environmental impact, for understanding AGN triggering and life cycles, and for calibrating galaxy feedback in cosmological models. We use the LOFAR Two-Metre Sky Survey (LoTSS) Data Release 1 catalogues to investigate this relationship. We cross-matched 8,745 radio-loud AGN with 0.08
| Original language | English |
|---|---|
| Journal | Astronomy & Astrophysics |
| Early online date | 10 Oct 2018 |
| DOIs | |
| Publication status | E-pub ahead of print - 10 Oct 2018 |
Keywords
- astro-ph.GA
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