{"total":10,"items":[{"citing_arxiv_id":"2607.02342","ref_index":6,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The VLA-COSMOS 3 GHz Large Project: Polarised source counts and catalogue","primary_cat":"astro-ph.GA","submitted_at":"2026-07-02T15:48:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Deep 3 GHz polarised source counts detect 65 sources (51 deg^{-2}), consistent with 1.4 GHz literature due to spectral index and depolarisation, with a 2σ upper limit of <2.0 deg^{-2} on polarised SFG density.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27812","ref_index":79,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Unraveling the Imprints of Fluctuation-dynamo on the Intracluster Medium with the SKA","primary_cat":"astro-ph.GA","submitted_at":"2026-06-26T07:54:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"MHD simulations indicate that SKA-Mid Band 5a can detect filamentary polarized emission from ICM magnetic fields at high resolution and sensitivity, allowing inference of turbulence driving scales.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27714","ref_index":23,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Fast Radio Bursts as Cosmological Probes","primary_cat":"astro-ph.CO","submitted_at":"2026-06-26T04:44:56+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"FRBs serve as cosmological probes via dispersion measure, scattering, and Faraday rotation to constrain baryon distribution, expansion history, magnetic fields, and fundamental physics effects.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25158","ref_index":257,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T20:45:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"SKAO will enable detection of synchrotron emission from prestellar cores to probe their magnetic field properties in nearby star-forming regions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13398","ref_index":8,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A robust super-time-stepping scheme for Ohmic and ambipolar diffusion","primary_cat":"astro-ph.IM","submitted_at":"2026-06-11T14:30:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A Runge-Kutta-Gegenbauer super-time-stepping method for stable, efficient handling of anisotropic non-ideal MHD diffusion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21281","ref_index":91,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Self-Consistent Parker Bound on Magnetic Monopoles","primary_cat":"hep-ph","submitted_at":"2026-05-20T15:12:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A self-consistent Parker bound on magnetic monopoles is derived using the galactic mean-field dynamo eigenmode and turbulent field seeding and acceleration, producing modified flux limits at low and intermediate masses that are robust to primordial magnetic fields.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.16917","ref_index":81,"ref_count":2,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky","primary_cat":"astro-ph.GA","submitted_at":"2026-05-16T10:13:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"SPICE-RACS DR2 delivers the largest single Faraday rotation measure catalog from a radio survey, with 250,000-340,000 RMs across most of the sky at median uncertainty of 2 rad m^{-2}.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.01277","ref_index":105,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Lights, Camera, Axion: Tracing Axions from Supernovae in the Diffuse $\\gamma$-ray Sky","primary_cat":"hep-ph","submitted_at":"2026-04-01T18:00:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Axions produced in supernovae generate a diffuse gamma-ray signal through conversion in magnetic fields, yielding competitive constraints on the axion-photon coupling from COMPTEL, EGRET, and Fermi-LAT data plus forecasts for future MeV telescopes.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"52 (2014) 415 [1403.0007]. [103] S. Ekstr¨ om and C. Georgy,Stellar evolution through the red supergiant phase, Galaxies 13 (2025) 81. [104] V. Heesen, T.-L. Klocke, M. Br¨ uggen, F. Tabatabaei, A. Basu, R. Beck et al., Nearby galaxies in the lofar 22 two-metre sky survey-ii. the magnetic field-gas relation , Astronomy & Astrophysics 669 (2023) A8. [105] R. Beck, Magnetic fields in spiral galaxies , The Astronomy and Astrophysics Review 24 (2015) 4 [1509.04522]. [106] V. Heesen, R. Beck, M. Krause and R.-J. Dettmar, Cosmic rays and the magnetic field in the nearby starburst galaxy NGC253 III. Helical magnetic fields in the nuclear outflow , Astron. Astrophys. 535 (2011) A79 [1109.0255]. [107] B. Adebahr, M."},{"citing_arxiv_id":"2603.05084","ref_index":16,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Distinguishability of magnetic massive black holes from environmental mimics with inspiral gravitational waves","primary_cat":"gr-qc","submitted_at":"2026-03-05T11:56:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Magnetic field corrections to inspiral waveforms appear at -2 PN and -3 PN orders and mimic power-law environmental gravity but can be distinguished above a transition density of about 10^{-4} kg/m^3 for Bonnor-Melvin cases using multi-event statistics.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.08025","ref_index":1,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"On the contribution of galaxies to the magnetic field in cosmic voids","primary_cat":"astro-ph.CO","submitted_at":"2025-10-09T10:02:15+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Superposition of static galactic magnetic dipoles is screened by intergalactic plasma and cannot account for lower bounds on magnetic fields in cosmic voids from blazar gamma-ray data.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}