{"total":13,"items":[{"citing_arxiv_id":"2606.27812","ref_index":93,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"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":"2606.25689","ref_index":6,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Tracing the Star Formation History of the Universe through Thermal Free-Free Emission with the SKA","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T10:57:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations of an SKA-Mid survey predict detection of 1.5e4 star-forming galaxies to z~7 with thermal SFR uncertainties of 0.1 dex, enabling constraints on cosmic star formation rate density.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25081","ref_index":217,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cosmology from Clustering of Continuum Galaxies","primary_cat":"astro-ph.CO","submitted_at":"2026-06-23T18:41:13+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Forecasts angular clustering for a 20,000 sq deg SKAO radio continuum survey reaching O(300-400 million) sources and discusses needed corrections for telescope systematics and population modeling.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.13391","ref_index":24,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Feedback in Extragalactic Star Clusters (FEAST): Spectral Energy Distributions and the Physical Properties of Star Clusters in NGC 628 with CIGALE","primary_cat":"astro-ph.GA","submitted_at":"2026-06-11T14:23:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"SED fitting of star clusters in NGC 628 identifies an evolutionary sequence from embedded young clusters to visible ones with a photo-dissociation region clearing timescale of approximately 4 Myr.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.02717","ref_index":3,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The Radio-IR Correlation in the Context of Deep Radio Source Counts","primary_cat":"astro-ph.GA","submitted_at":"2026-06-01T18:00:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A radio-luminosity-based model of mild q decrease to z~2 from cosmic ray losses mitigates the >3σ discrepancy in MeerKAT source counts near 10 μJy with ≥2σ evidence, while bounding intrinsic scatter.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.01957","ref_index":11,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Radio Continuum Emission from Evolving Star-Forming Galaxies -- I. Correlations Involving the Total Synchrotron Luminosity","primary_cat":"astro-ph.GA","submitted_at":"2026-06-01T09:16:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Simulations of evolving galaxies show strong L_nu-SFR and L_nu-V_rot correlations up to z~3, with turbulent magnetic fields dominating at low redshift and large-scale fields growing in importance at higher redshift.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.19658","ref_index":46,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs","primary_cat":"astro-ph.GA","submitted_at":"2026-05-19T10:51:35+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Multi-scale radio observations of 15 local U/LIRGs decompose emission to show nuclear components contribute ~50% on average while diffuse SF-related emission dominates ~80% of total power, with radio excess linked to AGN rather than boosted star formation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.05298","ref_index":31,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Kinematic Stratification in Extremely Red Quasars Revealed by JWST","primary_cat":"astro-ph.GA","submitted_at":"2026-05-06T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"JWST observations of ERQs show stratified gas kinematics via deblended optical emission lines, with UV lines dominated by scattered light and optical lines mixing scattered and obscured emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.01000","ref_index":9,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Prospects for Observing Galaxy Spectral Energy Distribution from the Radio to the far-Infrared in the Era of Next-Generation Radio Telescopes","primary_cat":"astro-ph.GA","submitted_at":"2026-05-01T18:06:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Simulations predict ngVLA at 100 GHz can detect galaxies above 10^9 solar masses at any redshift while SKA low frequencies reach massive dusty galaxies to z=5-7.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"2020), Matplotlib (Hunter 2007) APPENDIX radio-FIR Galaxy SED Reloaded21 T able 3.Number counts for each redshift and mass bin of the JAGUAR mock catalog [Ml,M u)\\(zl,zu] :z mean (0.0,1.760]:1.057 (1.760,2.689]:2.207 (2.689,3.628]:3.140 (3.628,4.647]:4.109 [6,7) 718455 375592 289299 239316 [7,8) 197283 131198 107669 87805 [8,9) 56930 44888 38595 30230 [9,10) 17247 12307 9666 6612 [10,11) 5540 1738 508 126 [11,∞) 279 112 15 4 Mchar 8584 5327 4882 4260 (4.647,5.789]:5.177 (5.789,7.094]:6.384 (7.094,8.606]:7.739 (8.606,10.378]:9.263 (10.378,12.480]:11.093 (12.480,15.0]:13.221 197319 149282 95882 32756 6756 865 60721 37565 19330 5188 764 67 17189 8435 3348 614 67 2 2662 870 176 18 0 0 27 1 1 0 0 0 1 0 0 1 0 0"},{"citing_arxiv_id":"2604.20950","ref_index":89,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Revisiting radio synchrotron diagnostics in star-forming galaxies","primary_cat":"astro-ph.GA","submitted_at":"2026-04-22T18:00:00+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Advection-only galactic wind models fail to reproduce observed vertical radio profiles without unrealistic velocities, synchrotron spectra are biased toward young electrons in dense regions, and bremsstrahlung/Coulomb losses cannot be neglected even when subdominant.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.19896","ref_index":161,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"HI 21-cm absorption in low- and high-excitation radio-loud AGNs at $z<0.5$ from MALS","primary_cat":"astro-ph.GA","submitted_at":"2026-04-21T18:20:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Five new HI 21-cm absorption detections in LERGs and HERGs at z<0.5 reveal disturbed gas kinematics with velocity offsets over 350 km/s and a 3% detection rate consistent with lower-redshift samples.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.18950","ref_index":6,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Very Long Baseline Interferometry Search for Nuclear Radio Continuum Emission in the Barred Spiral Galaxy NGC 7479","primary_cat":"astro-ph.GA","submitted_at":"2026-04-21T01:00:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"VLBI observations resolve NGC 7479's nucleus into two radio components separated by ~30 mas with an apparent change in separation over a decade, suggesting relativistic jet motion or nuclear wind shocks.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"2021), surrounded by young star formation regions in a shock front morphology. A rough upper estimate on the star formation rate in the bar region due to the jet-like feature is obtained by using the inte- grated 21-cm flux density from S. Laine & S. T. Gottesman (1998) as a substitute for the 20- cm integrated flux density and the relationship from E. F. Bell (2003; see also E. J. Murphy et al. 2011). Using this integrated flux density and this relationship, we compute a star for- mation rate of 2.7 M ⊙ yr−1 in the bar region. On the sky these \"jets\" appear as \"S\"-shaped arms, contrasting to the \"Z\"-shaped stellar spi- ral arms (as seen in Figure 1). Overall, the large-scale radio continuum struc- ture in NGC 7479 is reminiscent of the one seen"},{"citing_arxiv_id":"2511.13811","ref_index":5,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Steady-State or Not? The Evolution of Cosmic Ray Electron Spectra in Galaxies","primary_cat":"astro-ph.GA","submitted_at":"2025-11-17T19:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Time-dependent cosmic ray electron spectra in a simulated galactic disk match steady-state solutions up to 500 GeV but become steeper and more disk-confined at higher energies due to recent injections.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}