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F. Sweijen

Identifiers

  • name variant F. Sweijen 0.60 · backfill

Papers (21)

  1. Polarisation and Faraday rotation measure imaging at metre wavelengths with sub-arcsecond resolution: a foundational calibration strategy astro-ph.IM · 2026 · author #8
  2. A population-based approach to understanding radio AGN feedback with LOFAR: The LoTSS Deep Fields astro-ph.GA · 2026 · author #2
  3. The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11 astro-ph.CO · 2026 · author #10
  4. Scalable and robust wide-field facet calibration with LOFAR's longest baselines astro-ph.IM · 2025 · author #9
  5. The Crab Nebula at subarcsecond resolution with the International LOFAR Telescope astro-ph.HE · 2025 · author #3
  6. Unlocking ultra-deep wide-field imaging with sidereal visibility averaging astro-ph.IM · 2025 · author #6
  7. The LOFAR Two-metre Sky Survey: Deep Fields Data Release 2. I. The ELAIS-N1 field astro-ph.CO · 2025 · author #32
  8. A hidden Active Galactic Nuclei population: the first radio luminosity functions constructed by physical process astro-ph.GA · 2024 · author #6
  9. Into the depths: Unveiling ELAIS-N1 with LOFAR's deepest sub-arcsecond wide-field images astro-ph.IM · 2024 · author #3
  10. The first high-redshift cavity power measurements of cool-core galaxy clusters with the International LOFAR Telescope astro-ph.CO · 2024 · author #6
  11. Nuclear regions as seen with LOFAR international baselines: A high-resolution study of the recurrent activity astro-ph.GA · 2023 · author #3
  12. VLBI Imaging of high-redshift galaxies and protoclusters at low radio frequencies with the International LOFAR Telescope astro-ph.GA · 2023 · author #5
  13. V-LoTSS: The Circularly-Polarised LOFAR Two-metre Sky Survey astro-ph.GA · 2022 · author #44
  14. Identifying active galactic nuclei via brightness temperature with sub-arcsecond International LOFAR Telescope observations astro-ph.GA · 2022 · author #2
  15. Measuring cavity powers of active galactic nuclei in clusters using a hybrid X-ray-radio method -- A new window on feedback opened by subarcsecond LOFAR-VLBI observations astro-ph.CO · 2022 · author #6
  16. The LOFAR Two-metre Sky Survey -- V. Second data release astro-ph.GA · 2022 · author #98
  17. Pushing subarcsecond resolution imaging down to 30 MHz with the trans-European International LOFAR Telescope astro-ph.GA · 2021 · author #7
  18. Origin of the ring structures in Hercules A -- Sub-arcsecond 144 MHz to 7 GHz observations astro-ph.GA · 2021 · author #16
  19. Sub-arcsecond imaging with the International LOFAR Telescope I. Foundational calibration strategy and pipeline astro-ph.IM · 2021 · author #4
  20. Realising the LOFAR Two-Metre Sky Survey -- using the supercomputer JUWELS at the Forschungszentrum J\"ulich astro-ph.IM · 2019 · author #6
  21. SHARP -- VI. Evidence for CO (1-0) molecular gas extended on kpc-scales in AGN star forming galaxies at high redshift astro-ph.GA · 2019 · author #11

Mentions

  • 2508.12115 #9 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2506.19460 #3 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2501.04093 #32 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2501.07374 #6 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2411.05069 #6 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2407.13247 #3 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2403.03242 #6 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2311.12114 #3 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2306.00071 #5 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2212.09815 #44 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2207.05088 #6 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2207.13096 #2 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2202.11733 #98 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2108.07287 #16 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2108.07286 #7 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2108.07283 #4 · arxiv_oai · confidence 0.70 F. Sweijen
  • 1905.06363 #11 · arxiv_oai · confidence 0.70 F. Sweijen
  • 1910.13835 #6 · arxiv_oai · confidence 0.70 F. Sweijen
  • 2606.18333 #8 · arxiv_oai · confidence 0.70 F. Sweijen

Frequent Coauthors