{"total":38,"items":[{"citing_arxiv_id":"2606.28293","ref_index":37,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Accretion-Driven Evolution of Compact-Object Populations in Gas-Rich Environments and the Origin of Massive Gravitational-Wave Sources","primary_cat":"astro-ph.HE","submitted_at":"2026-06-26T17:38:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Accretion laws with super-linear mass dependence produce divergent population evolution that broadens compact-object mass distributions and drives binary mass ratios toward unity, providing a pathway to massive gravitational-wave sources.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26914","ref_index":81,"ref_count":1,"confidence":0.88,"is_internal_anchor":true,"paper_title":"Transforming X-ray Binary Astrophysics with SKA+VLBI","primary_cat":"astro-ph.HE","submitted_at":"2026-06-25T11:52:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"SKA+VLBI will deliver microarcsecond astrometry, polarimetry, and rapid multi-frequency imaging to track jets and accretion in X-ray binaries on AU scales.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26288","ref_index":129,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Constraints on Binarity for the Extreme Oe Variable Star AzV 493","primary_cat":"astro-ph.SR","submitted_at":"2026-06-24T18:35:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Chandra and spectroscopic observations of AzV 493 produce an X-ray luminosity upper limit of <2.5e33 erg/s and inconclusive RV variations, leaving binarity unconfirmed.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25995","ref_index":169,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"The evolution of the galaxy gas-phase mass-metallicity relation from $z=15$ to $z=0$ in the COLIBRE cosmological simulations","primary_cat":"astro-ph.GA","submitted_at":"2026-06-24T16:07:47+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"COLIBRE simulations find the galaxy gas-phase MZR already in place at z≈10 with little evolution until z≈5, then shallowens at low z, with high-mass turnover set by AGN feedback and low-mass end by core-collapse supernovae.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.22619","ref_index":121,"ref_count":1,"confidence":0.98,"is_internal_anchor":true,"paper_title":"Comparative Study of Two Luminous Red Novae I. 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We simi- larly define perturbations to the post-shock fluid veloc- ity, density, and pressure by generalizing Equation (12) to v = Vsh [f0 (ξ) + f1 (ξ, τ)] , (15) ρ = ρi \u0012 Rsh ri \u0013−n [g0 (ξ) + g1 (ξ, τ)] , (16) p = ρi \u0012 Rsh ri \u0013−n Vsh 2 [h0 (ξ) + h1 (ξ, τ)] . (17) Inserting these definitions into Equations (3)-(5) then yields a set of six equations - three zeroth-order and three first-order - where the zeroth-order equations are the self-similar equations from C23. We include all equa- tions in Appendix A.1. At the shock front ( ξ = 1) the shock jump condi-"},{"citing_arxiv_id":"2605.03128","ref_index":109,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Double Neutron Star Delay Times Across Cosmic Metallicities: The Role of Helium Star Progenitors","primary_cat":"astro-ph.SR","submitted_at":"2026-05-04T20:10:59+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":"2605.02998","ref_index":31,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The SRG/eROSITA diffuse soft X-ray background II. spectra and morphology of the eROSITA bubbles in the western Galactic hemisphere","primary_cat":"astro-ph.HE","submitted_at":"2026-05-04T18:00:00+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Spectra 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