{"total":16,"items":[{"citing_arxiv_id":"2606.30757","ref_index":69,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T18:00:52+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"SKAO continuum surveys will detect radio emission from JWST AGN and LRDs and distinguish between Compton-thick absorption, intrinsically weak accretion, and dense gas cocoon scenarios.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.30253","ref_index":73,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"No evolution in the number density of little red dots from cosmic dawn to cosmic noon","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T13:03:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Number density of LRDs with L_bol ≳ 3×10^44 erg s^{-1} shows no evolution at z>2 and is ~350 times higher than model predictions at cosmic noon.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27427","ref_index":52,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"SEEDZ: Rapid Galaxy Assembly as a Pathway to Supermassive Stars, Dense Stellar Environments and Massive Black Hole Seeds","primary_cat":"astro-ph.GA","submitted_at":"2026-06-25T18:00:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Rapid halo growth in SEEDZ simulations enables heavy black hole seed formation via supermassive stars at a comoving number density of 0.1 cMpc^{-3} by z=10, with most seeds in near-solar metallicity gas.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.07730","ref_index":87,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The X-ray-to-UV relation does not evolve in homogeneous quasar samples","primary_cat":"astro-ph.HE","submitted_at":"2026-06-05T17:53:58+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A bias-controlled quasar sample of ~2000 objects demonstrates that the X-ray-to-UV luminosity relation remains constant from redshift 0.7 to 5.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.03414","ref_index":15,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Hidden-sector accretion and warped black-string seeds for high-redshift supermassive black holes","primary_cat":"astro-ph.CO","submitted_at":"2026-06-02T09:58:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A warped 5D geometry with hidden-sector accretion produces growing Schwarzschild/Vaidya black-hole seeds on our brane via a common horizon intersection.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21589","ref_index":55,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A Magnetized Black Hole Envelope Model for Little Red Dots","primary_cat":"astro-ph.GA","submitted_at":"2026-05-20T18:00:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A theoretical model of a magnetized black hole envelope is developed to explain the broad emission lines and X-ray faintness observed in little red dots using co-rotating plasma clumps and limited X-ray sources.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.21574","ref_index":112,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"(LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample","primary_cat":"astro-ph.GA","submitted_at":"2026-05-20T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The survey identifies 27 low-redshift LRDs with compact morphology, V-shaped continua, broad Balmer lines with extreme decrements, and ubiquitous outflows, matching high-z counterparts and yielding a number density lower limit of 7.5e-10 cMpc^-3.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.14233","ref_index":76,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"A new sample of Little Red Dots at $z<0.45$ in DESI DR1: Broad Balmer lines, low ionization spectrum and no variability","primary_cat":"astro-ph.GA","submitted_at":"2026-05-14T00:59:21+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Eight low-redshift Little Red Dots identified in DESI DR1 exhibit broad Balmer lines, steep decrements, compact shapes, and negligible variability, with a number density roughly 10,000 times lower than at z>4.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.12141","ref_index":100,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Non-LTE atmosphere models of very luminous sources and their applicability to Little Red Dots, quasi-stars, and similar objects","primary_cat":"astro-ph.GA","submitted_at":"2026-05-12T14:01:48+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Non-LTE wind atmosphere models computed with CMFGEN reproduce the SED and Balmer decrement of most Little Red Dots when dust-attenuated with Av ~2, while predicting Fe II, O I, and Ca lines, but struggle to produce both a genuine Balmer break and strong lines simultaneously.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06791","ref_index":20,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"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":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.14535","ref_index":45,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe","primary_cat":"astro-ph.HE","submitted_at":"2026-04-16T02:04:33+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"High-redshift AGN emitting UHE protons up to 10^19 eV generate a 50 PeV cosmogenic neutrino bump consistent with IceCube data from their JWST-measured average properties without fine-tuning.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"for Early Galaxy and SMBH Assembly, Astrophys. J. 991, 37 (2025). [43] V. Kokorevet al., A Census of Photometrically Selected Little Red Dots at 4<z<9 in JWST Blank Fields, Astrophys. J.968, 38 (2024). [44] R. P. Naiduet al., A \"Black Hole Star\" Reveals the Re- markable Gas-Enshrouded Hearts of the Little Red Dots, arXiv e-prints (2025), arXiv:2503.16596 [astro-ph.GA]. [45] V. Rusakovet al., Little red dots as young supermassive black holes in dense ionized cocoons, Nature649, 574 (2026), arXiv:2503.16595 [astro-ph.GA]. [46] R. Kuze, K. Ioka, K. Murase, S. S. Kimura, and K. Inayoshi, Little Red Dots as Hidden Neu- trino Sources, arXiv e-prints 10.48550/arXiv.2601.11203 (2026), arXiv:2601.11203 [astro-ph.HE]. [47] C. M."},{"citing_arxiv_id":"2603.10162","ref_index":95,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The X-ray weakness of Little Red Dots and JWST-selected AGN: comparison with local AGN in different accretion regimes","primary_cat":"astro-ph.GA","submitted_at":"2026-03-10T18:54:51+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"High-z LRDs and JWST AGN exhibit X-ray weakness consistent with local super-Eddington accreting SMBHs, supporting a link to highly accreting systems across cosmic time.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.12548","ref_index":79,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\\sim4$","primary_cat":"astro-ph.GA","submitted_at":"2026-02-13T02:56:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Spectroscopic study of 11 LRDs at z~4 finds AGN origin for optical emission via broad Hα correlations and introduces a clumpy envelope model with growth timescales of 10^5-10^7 years.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.06954","ref_index":67,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Spectral Appearance of Self-gravitating Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots","primary_cat":"astro-ph.HE","submitted_at":"2026-02-06T18:51:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Self-gravitating disks heated by stars reach a universal optical effective temperature of 4000-4500 K independent of accretion rate, black hole mass, and viscosity, explaining Little Red Dots.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.02702","ref_index":96,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation","primary_cat":"astro-ph.GA","submitted_at":"2026-02-02T19:13:11+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"UV-bright companions to Little Red Dots provide Lyman-Werner fluxes of J21 ~ 10^2.5-10^5 that can suppress H2 cooling and enable direct collapse to massive black holes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2509.19422","ref_index":122,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts","primary_cat":"astro-ph.GA","submitted_at":"2025-09-23T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Coevolving super-Eddington black holes and nuclear starbursts in high-redshift halos naturally generate the V-shaped UV-to-optical spectra and weak high-energy emission of little red dots.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}