pith. sign in

Title resolution pending

The halo magnetic field of a spiral galaxy at z = 0 · DOI 10.1051/0004-6361/202453502

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
open at publisher browse 2 citing papers

Title metadata for this work has not finished resolving. The hub is built from the citation graph; the title resolver retries DOI and OpenAlex on its next pass.

fields

astro-ph.GA 2

years

2026 2

verdicts

UNVERDICTED 2

representative citing papers

Magnetised CGM Gas at z~1 revealed by SPICE-RACS

astro-ph.GA · 2026-05-16 · unverdicted · novelty 6.0

A 4.5σ excess RM dispersion of 4.13 ± 0.91 rad m^{-2} is found in 191 Mg II sightlines versus controls, implying model-dependent CGM magnetic fields of 0.4-0.8 μG at projected radii 20-150 kpc and z~1.14.

citing papers explorer

Showing 2 of 2 citing papers.

  • Magnetised CGM Gas at z~1 revealed by SPICE-RACS astro-ph.GA · 2026-05-16 · unverdicted · none · ref 155

    A 4.5σ excess RM dispersion of 4.13 ± 0.91 rad m^{-2} is found in 191 Mg II sightlines versus controls, implying model-dependent CGM magnetic fields of 0.4-0.8 μG at projected radii 20-150 kpc and z~1.14.

  • Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies astro-ph.GA · 2026-06-23 · unverdicted · none · ref 31

    Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.