{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:4Q37PQXO5HMOHRJNAMOMTXWXJB","short_pith_number":"pith:4Q37PQXO","schema_version":"1.0","canonical_sha256":"e437f7c2eee9d8e3c52d031cc9ded74844dfeb71ba6bcb6779849273c562d5ca","source":{"kind":"arxiv","id":"1510.03093","version":3},"attestation_state":"computed","paper":{"title":"Inner disk clearing around the Herbig Ae star HD\\,139614: Evidence for a planet-induced gap ?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Carmona, A. Crida, A. Matter, B. Lopez, J.-B. Le Bouquin, J.-C. Augereau, J.F. Gonzalez, J. Kluska, J. Olofsson, L. Labadie, W. F. Thi","submitted_at":"2015-10-11T20:08:51Z","abstract_excerpt":"Spatially resolving the inner dust cavity of the transitional disks is a key to understanding the connection between planetary formation and disk dispersal. The disk around the Herbig star HD 139614 is of particular interest since it presents a pretransitional nature with an au-sized gap, in the dust, that was spatially resolved by mid-IR interferometry. Using new NIR interferometric observations, we aim to characterize the 0.1-10~au region of the HD~139614 disk further and identify viable mechanisms for the inner disk clearing. We report the first multiwavelength radiative transfer modeling o"},"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":"1510.03093","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2015-10-11T20:08:51Z","cross_cats_sorted":[],"title_canon_sha256":"185fa826514bcb586f558bb65ba4a98be378bced991302d58f22ec2cefd790f4","abstract_canon_sha256":"4f614935d6079df62bf26885df0196d079c88f6b001b30806f8a042debffe724"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:22:35.476256Z","signature_b64":"4jcbfUfjHYPmEN+BbU+CYm8rluXmWg/PlTwu/u0TFDeT8eLuEuIc5C1cv5tGDz4a5fPI6iyLzEXywU+KIRV5AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e437f7c2eee9d8e3c52d031cc9ded74844dfeb71ba6bcb6779849273c562d5ca","last_reissued_at":"2026-05-18T01:22:35.475786Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:22:35.475786Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inner disk clearing around the Herbig Ae star HD\\,139614: Evidence for a planet-induced gap ?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Carmona, A. Crida, A. Matter, B. Lopez, J.-B. Le Bouquin, J.-C. Augereau, J.F. Gonzalez, J. Kluska, J. Olofsson, L. Labadie, W. F. Thi","submitted_at":"2015-10-11T20:08:51Z","abstract_excerpt":"Spatially resolving the inner dust cavity of the transitional disks is a key to understanding the connection between planetary formation and disk dispersal. The disk around the Herbig star HD 139614 is of particular interest since it presents a pretransitional nature with an au-sized gap, in the dust, that was spatially resolved by mid-IR interferometry. Using new NIR interferometric observations, we aim to characterize the 0.1-10~au region of the HD~139614 disk further and identify viable mechanisms for the inner disk clearing. We report the first multiwavelength radiative transfer modeling o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.03093","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1510.03093","created_at":"2026-05-18T01:22:35.475871+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.03093v3","created_at":"2026-05-18T01:22:35.475871+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.03093","created_at":"2026-05-18T01:22:35.475871+00:00"},{"alias_kind":"pith_short_12","alias_value":"4Q37PQXO5HMO","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_16","alias_value":"4Q37PQXO5HMOHRJN","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_8","alias_value":"4Q37PQXO","created_at":"2026-05-18T12:29:05.191682+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.11026","citing_title":"MINDS survey of silicates in T Tauri disks: Correlation between dust and gas","ref_index":264,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB","json":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB.json","graph_json":"https://pith.science/api/pith-number/4Q37PQXO5HMOHRJNAMOMTXWXJB/graph.json","events_json":"https://pith.science/api/pith-number/4Q37PQXO5HMOHRJNAMOMTXWXJB/events.json","paper":"https://pith.science/paper/4Q37PQXO"},"agent_actions":{"view_html":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB","download_json":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB.json","view_paper":"https://pith.science/paper/4Q37PQXO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.03093&json=true","fetch_graph":"https://pith.science/api/pith-number/4Q37PQXO5HMOHRJNAMOMTXWXJB/graph.json","fetch_events":"https://pith.science/api/pith-number/4Q37PQXO5HMOHRJNAMOMTXWXJB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB/action/storage_attestation","attest_author":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB/action/author_attestation","sign_citation":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB/action/citation_signature","submit_replication":"https://pith.science/pith/4Q37PQXO5HMOHRJNAMOMTXWXJB/action/replication_record"}},"created_at":"2026-05-18T01:22:35.475871+00:00","updated_at":"2026-05-18T01:22:35.475871+00:00"}