{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:CBVKG5KEAOZIC2GVTR6SC5WLVN","short_pith_number":"pith:CBVKG5KE","schema_version":"1.0","canonical_sha256":"106aa3754403b28168d59c7d2176cbab4df6fddc98fb7c077c9d269286da2fa8","source":{"kind":"arxiv","id":"2606.26232","version":1},"attestation_state":"computed","paper":{"title":"Modeling the curved dust sublimation front in protoplanetary disks: a potential probe of midplane turbulence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"2), (2) University of Michigan, (3) Universidad de Guadalajara, (4) Instituto de Radioastronom\\'ia y Astrof\\'isica-UNAM), Ezequiel Manzo-Mart\\'inez (1, Jes\\'us Hern\\'andez (1), Nuria Calvet (2), Paola D'Alessio (4), Ramiro Franco-Hern\\'andez (3), Rosa M. Torres (3) ((1) Instituto de Astronom\\'ia-UNAM","submitted_at":"2026-06-24T18:00:02Z","abstract_excerpt":"We present a new approach to calculate the geometry and emission of the dust inner wall in disks around T Tauri stars. This calculation follows a self-consistent approach given the disk structure and adopts a density-dependent sublimation temperature for the dust. We built spectral energy distributions (SEDs) of disk models with curved walls around a $0.5\\,M_\\odot$ star, finding that the curved wall starts at a radius of $\\sim 0.11$ au and extends to $\\sim 0.38$ au. The dependence on mass accretion rate, dust settling, and disk inclination on the resulting SEDs is explored, as well as the impa"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2606.26232","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2026-06-24T18:00:02Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"49dd42a0e09cf3d38346c411b9c6bd53e1c5e9a9557aae8b17ba625eede8ac5a","abstract_canon_sha256":"9f5c0b5a37849557876424f9f842472d8d13be9acf96064b9aa10eb70b9d8f33"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-26T00:15:30.598601Z","signature_b64":"Y5sXMJxmiSMP893pw/dOOtg9jhjDIzXLwisDIhgWigNVZ+XfNcydDYES5lNDYjRyQtfYXbotkBn0jb9luJvGCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"106aa3754403b28168d59c7d2176cbab4df6fddc98fb7c077c9d269286da2fa8","last_reissued_at":"2026-06-26T00:15:30.598152Z","signature_status":"signed_v1","first_computed_at":"2026-06-26T00:15:30.598152Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modeling the curved dust sublimation front in protoplanetary disks: a potential probe of midplane turbulence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"2), (2) University of Michigan, (3) Universidad de Guadalajara, (4) Instituto de Radioastronom\\'ia y Astrof\\'isica-UNAM), Ezequiel Manzo-Mart\\'inez (1, Jes\\'us Hern\\'andez (1), Nuria Calvet (2), Paola D'Alessio (4), Ramiro Franco-Hern\\'andez (3), Rosa M. Torres (3) ((1) Instituto de Astronom\\'ia-UNAM","submitted_at":"2026-06-24T18:00:02Z","abstract_excerpt":"We present a new approach to calculate the geometry and emission of the dust inner wall in disks around T Tauri stars. This calculation follows a self-consistent approach given the disk structure and adopts a density-dependent sublimation temperature for the dust. We built spectral energy distributions (SEDs) of disk models with curved walls around a $0.5\\,M_\\odot$ star, finding that the curved wall starts at a radius of $\\sim 0.11$ au and extends to $\\sim 0.38$ au. The dependence on mass accretion rate, dust settling, and disk inclination on the resulting SEDs is explored, as well as the impa"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.26232","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2606.26232/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2606.26232","created_at":"2026-06-26T00:15:30.598224+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.26232v1","created_at":"2026-06-26T00:15:30.598224+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.26232","created_at":"2026-06-26T00:15:30.598224+00:00"},{"alias_kind":"pith_short_12","alias_value":"CBVKG5KEAOZI","created_at":"2026-06-26T00:15:30.598224+00:00"},{"alias_kind":"pith_short_16","alias_value":"CBVKG5KEAOZIC2GV","created_at":"2026-06-26T00:15:30.598224+00:00"},{"alias_kind":"pith_short_8","alias_value":"CBVKG5KE","created_at":"2026-06-26T00:15:30.598224+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN","json":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN.json","graph_json":"https://pith.science/api/pith-number/CBVKG5KEAOZIC2GVTR6SC5WLVN/graph.json","events_json":"https://pith.science/api/pith-number/CBVKG5KEAOZIC2GVTR6SC5WLVN/events.json","paper":"https://pith.science/paper/CBVKG5KE"},"agent_actions":{"view_html":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN","download_json":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN.json","view_paper":"https://pith.science/paper/CBVKG5KE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.26232&json=true","fetch_graph":"https://pith.science/api/pith-number/CBVKG5KEAOZIC2GVTR6SC5WLVN/graph.json","fetch_events":"https://pith.science/api/pith-number/CBVKG5KEAOZIC2GVTR6SC5WLVN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN/action/storage_attestation","attest_author":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN/action/author_attestation","sign_citation":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN/action/citation_signature","submit_replication":"https://pith.science/pith/CBVKG5KEAOZIC2GVTR6SC5WLVN/action/replication_record"}},"created_at":"2026-06-26T00:15:30.598224+00:00","updated_at":"2026-06-26T00:15:30.598224+00:00"}