{"total":10,"items":[{"citing_arxiv_id":"2606.30157","ref_index":45,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"CO snow lines are stabilised by the vertical transport of volatiles","primary_cat":"astro-ph.EP","submitted_at":"2026-06-29T11:33:04+00:00","verdict":"CONDITIONAL","verdict_confidence":"MODERATE","novelty_score":7.0,"formal_verification":"none","one_line_summary":"2D disc simulations with vertical volatile transport produce stable CO snow surface equilibria and eliminate limit-cycle behavior seen in 1D models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27289","ref_index":127,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Unveiling Complex Chemistry in Planet-forming Disks with the SKAO","primary_cat":"astro-ph.SR","submitted_at":"2026-06-25T17:07:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"SKA will detect emission from heavy molecules and prebiotic species in obscured disk regions to constrain initial chemical conditions for planet formation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26332","ref_index":135,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"DiskMINT-GARDEN: Self-consistent Models to Estimate Disk Masses","primary_cat":"astro-ph.EP","submitted_at":"2026-06-24T19:16:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"A new grid of disk models with grain-surface CO chemistry plus an ML inference tool produces gas mass estimates from ALMA observations that match independent dynamical and HD values without requiring extreme elemental depletion.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23815","ref_index":82,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Interpreting the scattering surface in protoplanetary disks","primary_cat":"astro-ph.EP","submitted_at":"2026-06-22T18:01:20+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Semi-analytical model links observed scattering-surface height to small-dust mass, yielding global mass fractions of order 10^{-3} consistent with modest grain growth in ten protoplanetary disks.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.11344","ref_index":191,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Planet formation at the inner edge of the dead zone II. Outbursts, rings, vortices, and suppression of planetesimal formation","primary_cat":"astro-ph.EP","submitted_at":"2026-06-09T18:22:44+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"2D radiation-hydrodynamical simulations find accretion outbursts unstable to Rossby-wave instability, forming vortices that suppress planetesimal formation until post-burst quiescence.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.10816","ref_index":5,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Analysis of the young disk around WRAY 15-1880: does it contain a primitive planetary system?","primary_cat":"astro-ph.SR","submitted_at":"2026-06-09T12:59:04+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A candidate 0.3-7.6 MJup companion is reported in the gap of the ~2.8 Myr pre-transitional disk around WRAY 15-1880, with an ALMA blob interpreted as a vortex at the m=1 Lindblad resonance.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.08859","ref_index":74,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Framework to Model Stellar Irradiated Disks with Frequency-dependent Absorption and Scattering Opacities in Athena++","primary_cat":"astro-ph.EP","submitted_at":"2026-06-07T22:25:37+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"A new implementation of radial rays and multigroup radiation transport in Athena++ for frequency-dependent stellar irradiation achieves 2-5% average temperature agreement with Monte Carlo benchmarks in hydrostatic disk models using 64 bands.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.02734","ref_index":21,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Formation of multiple dust rings and gaps in protoplanetary discs by a single migrating planet II: radiative discs and observational signatures","primary_cat":"astro-ph.EP","submitted_at":"2026-06-01T18:01:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Numerical experiments demonstrate that one migrating planet produces multiple long-lived dust rings and gaps in radiative discs through migration jumps, with cooling affecting jump count but not structure lifetime.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.30023","ref_index":135,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"An archival summary: 15 years of ALMA observations on disks and planet formation","primary_cat":"astro-ph.EP","submitted_at":"2026-05-28T14:42:40+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":1.0,"formal_verification":"none","one_line_summary":"ALMA observed 3933 independent coordinates in nearby star-forming regions for disks and planet formation, analyzed by sky location, frequency coverage, exposure time, spectral lines, and angular resolution.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.18332","ref_index":64,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Dust characterization of halos: The extended emission in protoplanetary disks","primary_cat":"astro-ph.EP","submitted_at":"2026-04-20T14:31:54+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Halos in Elias 2-24, IM Lup, and DM Tau hold 20-30% of total dust mass with cm-sized grains, helping resolve the disk mass-budget problem even though drift and growth timescales are shorter than disk ages.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null}],"limit":50,"offset":0}