{"total":26,"items":[{"citing_arxiv_id":"2605.18161","ref_index":151,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"SDSS-V: Revealing a weak accretion state in X-ray selected red quasars","primary_cat":"astro-ph.GA","submitted_at":"2026-05-18T10:05:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Red quasars are intrinsically X-ray weak with low alpha_OX values, tracing a distinct evolutionary stage of suppressed black hole accretion relative to stellar mass growth.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.17993","ref_index":84,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Nuclear Activity and Host Galaxy Properties of Low-Luminosity AGN Identified from VLA 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simulations classify L* galaxies by central BH-to-stellar-mass ratio and trace how merger history drives divergence in BH growth, star formation, and morphology, offering an explanation for the observed scatter and for MW/M31 differences.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.15555","ref_index":26,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"A VLBA-resolved Jet Associated with Super-Eddington Accretion in a Radio-loud Quasar at $z=3.4$","primary_cat":"astro-ph.GA","submitted_at":"2026-05-15T02:48:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"VLBA multi-frequency imaging resolves a collimated jet extending ~745 pc in the z=3.4351 super-Eddington radio-loud quasar ID830, with v ≳ 0.19c and viewing angle ≲ 79° but δ ~ 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comparable hotspots, and ~32% restarting/remnant behavior compared to bright FRIIs, revealing a highly diverse population where FRII dynamics occur at low powers.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06791","ref_index":76,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Hidden Monsters with SPHEREx I: A goldmine for heavily reddened quasars at cosmic noon","primary_cat":"astro-ph.GA","submitted_at":"2026-05-07T18:00:19+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":7.0,"formal_verification":"none","one_line_summary":"SPHEREx data confirm 77 new luminous heavily reddened quasars at 1.5<z<3.9 that are hot-dust poor relative to unobscured quasars, supporting a blow-out feedback 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sequence","primary_cat":"astro-ph.GA","submitted_at":"2026-04-14T18:36:21+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Panchromatic SED modeling yields SFRs with smaller offset and scatter than optical-only fits for starburst to post-starburst galaxies, while Prospector AGN torus models distinguish AGN but underpredict luminosities by an order of magnitude.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2603.02520","ref_index":19,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Observational Properties of Near-Maximally Spinning Supermassive Black Holes","primary_cat":"astro-ph.HE","submitted_at":"2026-03-03T02:09:58+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":4.0,"formal_verification":"none","one_line_summary":"GRMHD simulations at spins 0.9375 and 0.998 yield similar fluid properties 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