{"total":11,"items":[{"citing_arxiv_id":"2607.07814","ref_index":31,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Intensity fluctuations of radio halo in galaxy cluster: Insights from power spectrum estimation","primary_cat":"astro-ph.CO","submitted_at":"2026-07-08T18:01:17+00:00","verdict":"CONDITIONAL","verdict_confidence":"HIGH","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Angular power spectra of 610 MHz radio halos show excess power-law fluctuations only in Abell 2744, requiring multiplicative C_ℓ ∝ ℓ^{-3} structure atop an exponential profile and consistent with ICM turbulence.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.07750","ref_index":45,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Multi-Wavelength Signatures of a Giant Cometary Radio Halo in MACSJ0417-1154","primary_cat":"astro-ph.HE","submitted_at":"2026-07-08T11:28:23+00:00","verdict":"CONDITIONAL","verdict_confidence":"HIGH","novelty_score":6.0,"formal_verification":"none","one_line_summary":"MACSJ0417’s giant radio halo shows spectral steepening and radio–X-ray correlation consistent with turbulence from a 6:1 off-axis merger that preserved the cool core; pure hadronic models are energetically excluded.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.06346","ref_index":19,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Unravelling Turbulence and Magnetic Fields in Galaxy Clusters with SKA and XRISM","primary_cat":"astro-ph.HE","submitted_at":"2026-07-07T14:45:29+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":3.0,"formal_verification":"none","one_line_summary":"A research framework combining XRISM turbulent velocity maps with SKA rotation measure grids to break degeneracies between magnetic field strength and cosmic-ray energetics in galaxy clusters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.31503","ref_index":19,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Large-Scale Structure of the Universe through the SKA lenses","primary_cat":"astro-ph.CO","submitted_at":"2026-06-30T11:22:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"This review chapter summarizes the cosmic web's theoretical framework, recent radio observations of diffuse gas, and the expected impact of the SKA on detecting baryons in filaments and cluster outskirts.","context_count":1,"top_context_role":"background","top_context_polarity":"unclear","context_text":"M. Awad, N. I. Libeskind, and Y. Hoffman.Monthly Notices of the Royal Astronomical Society, 520:4712-4728, 2023. doi: 10.1093/mnras/stad383. J. Bagchi et al.ApJ, 844(1):25, July 2017. doi: 10.3847/1538-4357/aa7949. M. Balboni et al.A&A, 686:A5, June 2024. doi: 10.1051/0004-6361/202347965. J. D. Barrow, P. G. Ferreira, and J. Silk.Phys. Rev. Let., 78(19):3610-3613, May 1997. doi: 10.1103/PhysRevLett.78.3610. D. Batcheldor, A. Marconi, D. Merritt, and D. J. Axon.ApJL, 663:L85-L88, July 2007. doi: 10.1086/520518. D. Baumann et al.arXiv e-prints, 2009. URLhttps://arxiv.org/abs/0907.5424. L. Beduzzi et al.A&A, 678:L8, Oct. 2023. doi: 10.1051/0004-6361/202346784. L. Beduzzi et al.A&A, 690:A67, Oct. 2024."},{"citing_arxiv_id":"2606.27812","ref_index":131,"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":"2606.26562","ref_index":9,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The SKA View of the Sunyaev-Zeldovich Effect from Massive Cosmic Halos","primary_cat":"astro-ph.CO","submitted_at":"2026-06-25T03:19:26+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"The SKA will enable high-resolution, high-sensitivity observations of the thermal SZ effect in massive halos, capturing both pressure substructures and large-scale ICM emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25746","ref_index":99,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Exploring the physics of ram pressure stripping with radio continuum observations in the SKA era","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T12:15:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Perspective on using SKA-Low and SKA-Mid radio continuum to extend ram pressure stripping studies to southern clusters and z~0.5.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25077","ref_index":166,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Small-scale Magnetic Fields in the Milky Way and Nearby Galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T18:35:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"Review chapter summarizing the importance of small-scale galactic magnetic fields and proposing SKA observation strategies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.24738","ref_index":96,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Probing Merger Shocks in Galaxy Clusters in the SKA Era","primary_cat":"astro-ph.HE","submitted_at":"2026-06-23T16:01:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Review summarizing cluster merger shocks, radio relics from SKA pathfinders, and future SKA science cases for studying these phenomena.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04084","ref_index":66,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster","primary_cat":"astro-ph.GA","submitted_at":"2026-06-02T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Self-regulating AGN jets in MHD simulations of cool-core clusters yield realistic FRI radio morphologies viewed along the jet axis and account for frequency-independent lobe extents via 1-50 μG fields allowing both young and old electrons to radiate.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.20779","ref_index":39,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A MINOT-based Study of Gamma-ray emission from SPT-CL J2012-5649/Abell 3667","primary_cat":"astro-ph.HE","submitted_at":"2026-05-20T06:19:47+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"MINOT modeling of Abell 3667 predicts a hadronic 1–300 GeV flux of ~1.15e-10 cm^-2 s^-1 at 3.7 R500, matching Fermi-LAT, with ~76% of flux outside R500 and IC subdominant by ~20.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}