{"total":13,"items":[{"citing_arxiv_id":"2607.00105","ref_index":178,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"AGN radiative feedback as the main regulator of [O III] outflow activity and obscuration in X-ray AGN","primary_cat":"astro-ph.GA","submitted_at":"2026-06-30T19:45:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Higher Eddington ratio AGN exhibit increased [O III] outflow incidence and reduced obscuration, supporting radiative feedback as the regulator.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.00084","ref_index":47,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Little Red Dots at z~2 in EIGER reveal a gentle decline with respect to their peak number density at z~5","primary_cat":"astro-ph.GA","submitted_at":"2026-06-30T19:23:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Five LRDs at z≈2 yield number density ≈7×10^{-6} cMpc^{-3}, confirming a decline from the z≈5 peak but gentler than prior photometric estimates.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.29608","ref_index":56,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Lockman-SpReSO Project: A Deep X-ray Spectral View of a FIR-selected AGN Population","primary_cat":"astro-ph.GA","submitted_at":"2026-06-28T21:20:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"MODERATE","novelty_score":4.0,"formal_verification":"none","one_line_summary":"X-ray analysis of 94 FIR-selected AGNs at z=0.07-5 shows rising obscured fraction with redshift, soft excess in 10 sources, and a luminosity-dependent covering factor correlation supporting the receding torus model.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17144","ref_index":47,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Decoupled Kinematics and Excitation in the Compton-thick AGN NGC 6552: Spatially Resolved KOOLS-IFU Observations","primary_cat":"astro-ph.GA","submitted_at":"2026-06-15T18:00:02+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"IFU spectroscopy of NGC 6552 reveals decoupled ionized gas kinematics and excitation, with outflow energetics consistent with multi-phase outflow models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12511","ref_index":217,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Unification models of Active Galactic Nuclei","primary_cat":"astro-ph.GA","submitted_at":"2026-06-10T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":0.0,"formal_verification":"none","one_line_summary":"Overview chapter summarizing traditional orientation-based and radiation-regulated unification models for AGN, including evolutionary aspects and changing-look AGN.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.12076","ref_index":74,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population","primary_cat":"astro-ph.GA","submitted_at":"2026-06-10T13:41:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"After applying IR-informed priors to X-ray NH posteriors in a sample of 811 high-z AGN, CTK sources comprise 17% of the population at 3<z<6 with no significant evolution.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06578","ref_index":135,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A Disappearing Act: Constraints From \"Missing\" Flares of Repeating Partial TDE Candidates","primary_cat":"astro-ph.HE","submitted_at":"2026-06-04T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Non-detections of expected third flares in TDE 2022dbl and TDE 2020vdq support rpTDE interpretation over independent events, with modeling favoring bound main-sequence star orbits and deep initial encounters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.17547","ref_index":10,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Population synthesis of active galactic nuclei based on the radiation-regulated unification model","primary_cat":"astro-ph.HE","submitted_at":"2026-05-17T17:01:24+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Using ray-tracing simulations and simulation-based inference, the authors construct an AGN population that reproduces the cosmic X-ray background, number counts, and absorption properties, deriving an intrinsic Compton-thick fraction of 40±3%.","context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"70-monthSwift/BAT survey, obtained with optical spectroscopy. A22 constrained simultaneously the intrinsic (corrected for sur- vey and measurement biases) BHMF and ERDF in the local Uni- verse (z<0.3) for both unobscured (type 1) and obscured (type 2) AGNs. The A22 local BHMF,Φ 0(logM BH)= dN d logM BH withNbe- ing the number of sources, is described by a modified Schechter function: Φ0(logM BH)∝ln(10)Φ ∗ MBH M∗ !α+1 exp − MBH M∗ !β ,(1) whereM ∗ is in units of M ⊙,Φ ∗ is in units of Mpc −3 dex−2, and βchanges the slope of the cutoffat highM BH. The A22 local ERDF,ξ 0(logλ Edd)= dN d logλEdd , is described by a broken power- law: ξ0(logλ Edd)∝ξ ∗  λEdd λ∗ !δ1 + λEdd λ∗ !δ2 −1 ,(2) whereξ ∗ is in units of Mpc−3 dex−2 andδ 2 > δ1."},{"citing_arxiv_id":"2605.15263","ref_index":269,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"On the quenching of LRD X-ray emission by both Compton-thick gas and high accretion rates","primary_cat":"astro-ph.GA","submitted_at":"2026-05-14T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"LRDs require Compton-thick gas at moderate metallicity plus high accretion rates producing weak X-rays to explain their non-detection, implying they are not chemically pristine.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.13968","ref_index":63,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes","primary_cat":"astro-ph.HE","submitted_at":"2026-05-13T18:00:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"The cosmologically integrated neutrino emission from supermassive black hole coronae in Seyfert galaxies can account for the sub-PeV diffuse extragalactic neutrino flux observed by IceCube.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"αmpc2 ,L x, ¯M•(z)] (9) whereρ(z) is the number density of AGN X-ray sources, H(z) =H 0 √ (1 +z) 3ΩM + Ω Λ is the Hubble parameter, with Ω M≈0.3 and ΩΛ ≈0.7 for standard ΛCDM cos- mology, andH 0 = 70km s−1Mpc−1. The luminosityL ν is the source-dependent neutrino luminosity. We rely on the redshift-dependent modeling of the X- ray luminosity function (XLF) [63], necessary for an inte- gration of Eq. (9), and include contributions from galax- ies withL x >10 41 erg s−1(See Appendix C). The active SMBH mass function is unlikely to significantly affect the predicted diffuse neutrino flux (see§II). However, we still include it in our modeling to account for poten- tial contributions from sources with largeM •and low"},{"citing_arxiv_id":"2604.10942","ref_index":40,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Probing Active Galactic Nuclei and Measuring the Hubble constant with Extreme-Mass-Ratio Inspirals","primary_cat":"gr-qc","submitted_at":"2026-04-13T03:20:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Modeling accretion disk interactions with EMRIs allows reliable environment identification and boosts dark-siren Hubble constant precision by as much as 20% for individual events.","context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"Furthermore, as will be shown later, in the non-vacuum case, the dark siren method with luminosity weighting based on accretion disk parameters can further improve the precision of the Hubble constant measurement, com- pared with the vacuum case where only sky-localization weighting is used. In this dark siren analysis, we adopt the broad-line AGN catalog published by [40]. This catalog was uni- formly constructed from galaxies and quasars with exist- ing spectroscopic observations in SDSS DR7. It contains 14,584 AGNs within the redshift range ofz <0.35, covers a sky area of approximately 8200 deg2 (about 20% of the full sky), and is highly complete within the parent spectroscopic sample of SDSS DR7. Figure 5 illustrates"},{"citing_arxiv_id":"2510.18741","ref_index":240,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","primary_cat":"astro-ph.CO","submitted_at":"2025-10-21T15:46:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Relativistic N-body simulations of Lambda_s CDM produce a redshift-dependent crest in the matter power spectrum ratio, peaking at 20-25% near the transition and leaving a 15-20% uplift at z=0 on group scales.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"[238] A. van der Welet al., 3D-HST+CANDELS: The Evolu- tion of the Galaxy Size-Mass Distribution sincez = 3, Astrophys. J.788, 28 (2014), 1404.2844. [239] J. Airdet al., The NuSTAR Extragalactic Surveys: First Direct Measurements of the≳ 10 keV X-Ray Luminosity Function for Active Galactic Nuclei atz >0.1, Astrophys. J.815, 66 (2015), 1511.04184. [240] Y. Ueda, M. Akiyama, G. Hasinger, T. Miyaji, and M. G. Watson, Toward the Standard Population Syn- thesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations, Astrophys. J.786, 104 (2014), 1402.1836. [241] M. Kilbinger, Cosmology with cosmic shear observations:"},{"citing_arxiv_id":"2410.15523","ref_index":21,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"TeV to PeV neutrinos from AGN coronae","primary_cat":"astro-ph.HE","submitted_at":"2024-10-20T22:15:25+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"A Comptonization model of AGN coronae combined with Monte-Carlo photopion production and cosmological evolution can account for IceCube's ~100 TeV and sub-PeV neutrinos using only photohadronic processes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}