{"total":6,"items":[{"citing_arxiv_id":"2606.06226","ref_index":35,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A New Member of the Fast and Furious Family: A Relativistic and Time-Variable UV Outflow in a Luminous Quasar","primary_cat":"astro-ph.GA","submitted_at":"2026-06-04T14:36:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Detection of a time-variable relativistic UV outflow at velocities up to 0.3c in quasar J2318, with estimated mass-loss rate and kinetic luminosity above typical feedback thresholds.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.02074","ref_index":21,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts","primary_cat":"astro-ph.GA","submitted_at":"2026-06-01T11:02:05+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"The W cloud is reinterpreted as a disrupting galaxy group with a dynamically coherent tidal tail delivering low-mass star-forming dwarfs to the Virgo cluster.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2505.04694","ref_index":2,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cluster Lensing Mass Inversion (CLUMI+): Combining Dynamics and Weak Lensing around Galaxy Clusters","primary_cat":"astro-ph.CO","submitted_at":"2025-05-07T18:00:02+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":6.0,"formal_verification":"none","one_line_summary":"CLUMI+ jointly models weak and strong lensing with caustic escape-velocity data, recovering cluster mass profiles from core to infall without equilibrium assumptions.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2505.01710","ref_index":2,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"RVSNUpy: A Python Package for Spectroscopic Redshift Measurement Based on Cross-Correlation","primary_cat":"astro-ph.CO","submitted_at":"2025-05-03T06:17:31+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A new Python tool and template set show that the 40 km/s SDSS versus Hectospec redshift offset is caused by template velocity offsets, and calibrating templates to synthetic rest-frame spectra removes the offset.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2412.07834","ref_index":1,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Evidence that pre-processing in filaments drives the anisotropic quenching of satellite galaxies in massive clusters","primary_cat":"astro-ph.GA","submitted_at":"2024-12-10T19:00:01+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Using 11 CLASH clusters, this paper finds that satellite quenching is anisotropic out to at least 2.5 R200, peaking near 1.25 R200, and concludes pre-processing in large-scale structure, not AGN feedback, drives the signal.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2009.11925","ref_index":2,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Single magnetic white dwarfs with Balmer emission lines: A small class with consistent physical characteristics as possible signposts for close-in planetary companions","primary_cat":"astro-ph.SR","submitted_at":"2020-09-24T19:44:14+00:00","verdict":"ACCEPT","verdict_confidence":"HIGH","novelty_score":6.0,"formal_verification":"none","one_line_summary":"SDSS J121929.45+471522.8 is found to be the third isolated magnetic white dwarf with Zeeman-split Balmer emission, closely matching the other two known cases.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}