{"total":18,"items":[{"citing_arxiv_id":"2607.00921","ref_index":286,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Spatially resolved optical and mid-infrared spectroscopy of SDSS1335+0728: implications for the origin of the Ansky event","primary_cat":"astro-ph.GA","submitted_at":"2026-07-01T13:24:29+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Spatially resolved spectroscopy shows SDSS1335+0728 has a three-zone ionisation structure, optically thin dust, and sustained low-level nuclear activity for at least 1500 years, implying the Ansky event is a faint transient in an already accreting low-mass SMBH.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2607.00105","ref_index":101,"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":"2606.27675","ref_index":152,"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":"2606.23456","ref_index":265,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Stellar winds of O-type stars traced by high ionization fine-structure emission lines with JWST/MIRI","primary_cat":"astro-ph.SR","submitted_at":"2026-06-22T15:06:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"JWST/MIRI detects [Ne V] 14.3 micron emission from O-star winds in 5 of 22 observed stars, enabling wind speed and mass-loss rate estimates even in weak-wind regimes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20810","ref_index":41,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Investigating the Spectral Properties of Dual Nuclei in Galaxy Mergers from the GOTHIC survey: Supermassive Black Hole Growth, metal enrichment and Dual AGN","primary_cat":"astro-ph.GA","submitted_at":"2026-06-18T18:01:07+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Spectroscopic analysis of dual nuclei shows SMBH masses higher in galaxy mergers than single nuclei at fixed stellar mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.20360","ref_index":4,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Lightstack: A Python Package for Creating Photometric Data Cubes","primary_cat":"astro-ph.IM","submitted_at":"2026-06-18T15:23:19+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"lightstack is a Python package that creates photometric data cubes from standalone multi-band images via cropping, stacking, and PSF 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ETGs that match predictions from the multiple-population scenario linking the UV upturn to second-generation stars from dissolved globular clusters.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.04368","ref_index":67,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"A Planetary Nebula from a 5.7 $M_{\\odot}$ Progenitor in a 90 Myr M31 Star Cluster","primary_cat":"astro-ph.SR","submitted_at":"2026-06-03T02:33:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A PN in a 90 Myr M31 cluster is associated via position and velocity, implying a 5.66 solar mass progenitor with nitrogen enhancement.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.18973","ref_index":177,"ref_count":2,"confidence":0.88,"is_internal_anchor":true,"paper_title":"GRB 260310A/SN 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nuclei.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.03577","ref_index":242,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves","primary_cat":"astro-ph.GA","submitted_at":"2026-05-05T09:45:16+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Low-luminosity AGN exhibit structure function slopes rising from 0.1 to 0.3 with black hole mass, no breaks on decadal scales, amplitude anticorrelated with luminosity and positively correlated with mass.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.00988","ref_index":106,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Tidal pre-conditioning and ram-pressure stripping in NGC 1427A. Deep VLT/MUSE spectroscopy and FUV-to-radio observations trace a Fornax Cluster dwarf in transformation","primary_cat":"astro-ph.GA","submitted_at":"2026-05-01T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Multi-phase observations of NGC 1427A indicate tidal torquing from a dwarf fly-by has pre-conditioned its gas for ram-pressure stripping by the Fornax intracluster medium, placing the galaxy at the onset of environmental quenching with a declining star formation rate.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.26195","ref_index":129,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Resolved Maps of Gas and Dust in a Massive Quiescent Galaxy at z=2 from INQUEST-JWST: Evidence of Accretion and Rejuvenation","primary_cat":"astro-ph.GA","submitted_at":"2026-04-29T00:46:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Resolved gas and dust maps in a z=2 quiescent galaxy reveal accreted material from tidal interactions and a past star-formation rejuvenation, indicating that gas content variations are not solely due to consumption timescales.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2508.10987","ref_index":55,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"A massive and evolved slow-rotating galaxy in the early Universe","primary_cat":"astro-ph.GA","submitted_at":"2025-08-14T18:00:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"A massive quiescent galaxy at z=3.449 exhibits low rotation (λ_Re = 0.123) consistent with slow-rotator kinematics, indicating early formation of dispersion-dominated systems.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}