{"total":14,"items":[{"citing_arxiv_id":"2606.28171","ref_index":12,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Demographics of planet-forming disks with the SKAO","primary_cat":"astro-ph.EP","submitted_at":"2026-06-26T15:03:59+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"SKAO will enable the first large-scale high-resolution surveys of cm-wavelength disk emission to constrain dust growth, pebble demographics, and planet formation processes.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27535","ref_index":95,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Dust Mineralogy of Interstellar Comet 3I/ATLAS from JWST/MIRI Observations","primary_cat":"astro-ph.EP","submitted_at":"2026-06-25T20:32:42+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":8.0,"formal_verification":"none","one_line_summary":"JWST observations indicate that interstellar comet 3I/ATLAS has dust dominated by amorphous silicates similar to the ISM, unlike the crystalline silicate-rich dust in Solar System comets.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27278","ref_index":13,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Astrochemical Study of Early Embedded Disks","primary_cat":"astro-ph.SR","submitted_at":"2026-06-25T16:55:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"The paper proposes the iSEEDs project to integrate machine learning with astrochemistry for extracting physical conditions and molecular abundances from protostellar disk datasets.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25794","ref_index":126,"ref_count":2,"confidence":0.9,"is_internal_anchor":false,"paper_title":"Substructures in Planet-Forming Disks with the SKAO","primary_cat":"astro-ph.EP","submitted_at":"2026-06-24T13:13:23+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"This review chapter discusses open questions on protoplanetary disk substructures and how SKA-Mid continuum observations at 12.5 GHz can help resolve them.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.23794","ref_index":45,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"MINDS: Complementary inclinations in the binary system HK Tau reveal gas- and ice-phase chemistry","primary_cat":"astro-ph.EP","submitted_at":"2026-06-22T18:00:03+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Observations of the HK Tau binary with JWST reveal gas-phase molecular lines in the low-inclination primary and ice absorption features in the edge-on secondary, enabled by their differing inclinations.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.05132","ref_index":4,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): Formaldehyde (H$_2$CO) emission and its links to disk properties","primary_cat":"astro-ph.EP","submitted_at":"2026-06-03T17:37:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"ALMA survey detects H2CO in 45% of 20 disks and finds strong correlations of line luminosity with disk size, mass, and stellar luminosity, suggesting grain-surface formation.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.30023","ref_index":13,"ref_count":1,"confidence":0.9,"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":1,"top_context_role":"background","top_context_polarity":"background","context_text":"(*) Project codes with the same number of publications are ranked at the same position in the second column. References: (1) Andrews et al. (2018), (2) Huang et al. (2018a), (3) P' erez et al. (2016), (4) Pinilla et al. (2018b), (5) ¨Oberg et al. (2021), (6) Law et al. (2021), (7) Long et al. (2018a), (8) Long et al. (2019), (9) Manara et al. (2019), (10) ALMA Partnership et al. (2015), (11) Long et al. (2018c), (12) Mayama et al. (2018), (13) Keppler et al. (2019), (14) Isella et al. (2016), (15) P' erez et al. (2019), (16) Ansdell et al. (2016), (17) Kastner et al. (2018), (18) Qi et al. (2019), (19) van der Marel et al. (2019), (20) Ohashi et al. (2023a), (21) Fedele et al. (2018), (22) Andrews et al. (2016), (23) Pinilla et al. (2015b), (24) van der Marel et al. (2016), (25) Teague et al."},{"citing_arxiv_id":"2605.13445","ref_index":18,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"VLTI/PIONIER imaging of post-AGB binaries. An INSPIRING hunt for inner rim substructures in circumbinary discs","primary_cat":"astro-ph.SR","submitted_at":"2026-05-13T12:39:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"High-resolution interferometric imaging of eight post-AGB circumbinary discs reveals diverse inner-rim substructures including azimuthal brightness enhancements and arc-like features not explained by inclination alone.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.02769","ref_index":58,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"JWST high-contrast spectroscopy with speckle modelling: Atmospheric retrievals of the T dwarf companion HD 19467 B","primary_cat":"astro-ph.EP","submitted_at":"2026-05-04T16:09:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Joint speckle-atmosphere retrievals on JWST spectra of HD 19467 B and a field T dwarf detect H2O, CH4, CO, CO2 and NH3, yield carbon isotopic ratios of 154 and 85 respectively, and show near-solar metallicity with subsolar C/O.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.01955","ref_index":6,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"On the Dust Substructures Triggered by Two Super-Earths Migrating in Low-viscosity Disks","primary_cat":"astro-ph.EP","submitted_at":"2026-05-03T16:38:22+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Two migrating super-Earths in low-viscosity disks trigger narrow and broad dust substructures with high dust-to-gas ratios favorable for planetesimal formation.","context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"tional mesh and domain are the same as in Afkanpour et al. (2024) to facilitate the comparison of the planet evolution in the protoplanetary disks with gas and dust, considered in this work, with the purely gaseous disk. The standard outflow boundary conditions are applied at the disk boundaries. The wave killing-zones operate in the domains of [0.2R 0,0.268R 0] and [6.32R 0,7.0R 0] 1 The quantitiesaanbhave been corrected for the typos present in Auddy et al. (2022). Dust substructures triggered by two migrating super-Earths5 in the inner and outer boundaries, respectively (de Val- Borro et al. 2006). The planets are placed on circular orbits in the steady- state disk, described in the previous subsection. Their masses start from zero and grow to their final masses"},{"citing_arxiv_id":"2604.19246","ref_index":70,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The Ophiuchus DIsc Survey Employing ALMA (ODISEA). Substructures as a function of SED Class and disc mass in 100 systems","primary_cat":"astro-ph.EP","submitted_at":"2026-04-21T08:57:34+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"ALMA observations of 100 Ophiuchus discs show substructures linked to giant planet formation are common in discs above 10 Earth masses of dust and increase from Class I to Class II stages.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.18332","ref_index":25,"ref_count":1,"confidence":0.9,"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},{"citing_arxiv_id":"2604.09526","ref_index":5,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"High-Contrast Imaging of Forming Protoplanets: VLTs, JWST, and the Promise of ELT","primary_cat":"astro-ph.EP","submitted_at":"2026-04-10T17:46:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Reviews direct imaging of protoplanets and proposes deriving observational estimates of planet mass-to-radius ratio to test formation models, highlighting ELT capabilities.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"idea that embedded protoplanets shape their environments. Thus we are sensitive to a population of planets that can not currently be probed with other detection tech- niques (see Fig. 2). However, alternative explanations exist, such as iceline-induced dust traps or magnetohydrodynamic effects, complicating the overall picture and in- terpretation (see [5] for a comprehensive review). The inferred properties of putative protoplanets are strongly dependent on modeling assumptions, and degeneracies in simulations introduce significant uncertainties. This limits our ability to link specific structures to the presence of forming planets. Beyond morphology, another promising approach to inferring the presence of"},{"citing_arxiv_id":"2604.09011","ref_index":142,"ref_count":1,"confidence":0.9,"is_internal_anchor":false,"paper_title":"The formation of planetary systems: physics, populations, and architectures","primary_cat":"astro-ph.EP","submitted_at":"2026-04-10T06:23:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"The Bern Model has incorporated MHD disk evolution, pebble accretion, and improved interiors, yielding quantitative matches to exoplanet mass functions, radius distributions, and system architectures.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"In [97, 87], this approach has revealed the possibil- ity of multiple generations of planets being formed, shaped by different accretion mechanisms and migration patterns. 3.4 Disk structure The ubiquity of substructures in protoplanetary disks as revealed by ALMA [141] has altered our picture of the typical environment planets form in. Even though the origin of these substructures is still debated [142], they certainly have a huge impact on the planet formation process. This led many recent works to investigate the formation of planets at special locations in the disk. Some works consider smooth disks with localized rings of planetesimals [95, 143, 144, 145] while others model the observed the dust rings by modifying the structure of the gas disk [145, 146] or considering"}],"limit":50,"offset":0}