{"total":10,"items":[{"citing_arxiv_id":"2607.00105","ref_index":134,"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":"2606.31998","ref_index":172,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Radiation-pressure instability is an artifact of constant-$\\alpha$ closure","primary_cat":"astro-ph.HE","submitted_at":"2026-06-30T17:33:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Requiring thermal stability and single-valuedness in the thin-disk Ṁ-Σ plane produces a viscosity law α(X) with X = P_gas/P_rad that eliminates the radiation-pressure dominated instability while preserving the effective-temperature profile.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.28501","ref_index":102,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A hierarchical Bayesian framework for cosmology using Type 1 AGN variability","primary_cat":"astro-ph.CO","submitted_at":"2026-06-26T18:00:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A hierarchical Bayesian framework that uses the empirical anti-correlation between AGN variability amplitude and luminosity to infer cosmological parameters from moderate-baseline light curves via importance reweighting.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27675","ref_index":67,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"OzSSy1: The Australian Southern Seyfert-1 Spectroscopic Atlas and Catalogue at z < 0.1","primary_cat":"astro-ph.GA","submitted_at":"2026-06-26T03:13:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Presents a public spectroscopic atlas of 887 Southern broad-line AGNs at low redshift, including continuum decompositions and emission-line fits.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.24744","ref_index":115,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Unlocking the Full Potential of SKAO Extra-galactic Science with High-multiplex Optical Spectroscopy","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T16:08:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Optical spectroscopy is required to unlock the full potential of SKAO extragalactic surveys through precise redshifts, activity diagnostics, HI stacking, and large-scale structure mapping.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.21426","ref_index":104,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The Fundamental Planes of Black Hole Activity for High-Synchrotron-Peaked BL Lacertae Objects","primary_cat":"astro-ph.HE","submitted_at":"2026-06-19T13:45:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A sample of 69 HBLs yields intrinsic radio-X-ray correlation L_R,int ∝ L_X,int^0.68 and fundamental plane log L_R,int = 0.57 log L_X,int + 0.33 log M_BH + 12.65, consistent with synchrotron cooling model for X-ray emission.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.08782","ref_index":123,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe","primary_cat":"astro-ph.GA","submitted_at":"2026-06-07T18:58:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"JWST spectra reveal that two z~7 galaxies already show near-solar iron-to-silicon ratios with no strong odd-even effect, favoring early Type Ia supernovae over pair-instability supernovae as the source of iron enrichment.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.06578","ref_index":166,"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":"2605.17993","ref_index":111,"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 Observations","primary_cat":"astro-ph.GA","submitted_at":"2026-05-18T07:49:49+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"VLA radio-selected LLAGN show 84% optical, 63% X-ray, and 13% infrared detection rates, with black holes ~0.7 dex smaller, accretion rates ~4.2 dex lower, and host galaxies ~0.3 dex lower in stellar mass with ~0.5 dex suppressed star formation than Swift-BAT AGN.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2602.11093","ref_index":159,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method","primary_cat":"astro-ph.CO","submitted_at":"2026-02-11T18:01:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Galaxy cluster observations yield two preferred directions with cosmic anisotropy amplitude of about 5.3 times 10 to the minus 4 at roughly 1 sigma overall significance, though higher in the XMM-Newton subsample.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"and regional fitting method [86] can well reflect the anisotropy level of the local universe. SNe Ia observations reveal departures from isotropy at confidence levels from 1.4 to 4.7 σ [86, 91, 130, 131, 146, 158]. It is worth noting that the latest Pantheon+ SNe Ia are still not uniformly distributed in the sky; some SNe are very concentrated, forming a belt-like structure that is the SDSS sample [159]. A large number of researches have explored the impact of inhomogeneous distribution of SNe on the results of cosmic anisotropy, and found that the unevenness of the spatial distribution of samples will affect the preferred direction of anisotropy [160, 161] and contribute a certain level of anisotropy [86, 91]. To circumvent this problem, on the one hand, a subsample with uniform spatial distribution can be selected"}],"limit":50,"offset":0}