{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:4YKBJDSASNNMKZRTBD2QOK7CLO","short_pith_number":"pith:4YKBJDSA","schema_version":"1.0","canonical_sha256":"e614148e40935ac5663308f5072be25bae1b0beadcc929ae485c5a46b675910f","source":{"kind":"arxiv","id":"1512.02276","version":1},"attestation_state":"computed","paper":{"title":"Monte-Carlo radiative transfer simulation of the circumstellar disk of the Herbig Ae star HD 144432","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Kreplin, D. Schertl, F. Malbet, F. Massi, G. Weigelt, K.-H. Hofmann, L. Chen, Ph. Stee, R. Petrov","submitted_at":"2015-12-07T22:48:16Z","abstract_excerpt":"Studies of pre-transitional disks, with a gap region between the inner infrared-emitting region and the outer disk, are important to improving our understanding of disk evolution and planet formation. Previous infrared interferometric observations have shown hints of a gap region in the protoplanetary disk around the Herbig Ae star HD~144432. We study the dust distribution around this star with two-dimensional radiative transfer modeling. We compare the model predictions obtained via the Monte-Carlo radiative transfer code RADMC-3D with infrared interferometric observations and the {\\SED} of H"},"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":"1512.02276","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-12-07T22:48:16Z","cross_cats_sorted":[],"title_canon_sha256":"e859fa6d3e5beb637b7dd76c4fab4286f9c35ee9d337e52e3badc9e5d34eee83","abstract_canon_sha256":"24e38261bc339d38ba5eb47aeee61e1c4a87e622e11c77c7a2cf55252f2c74e5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:21:26.125645Z","signature_b64":"Tg87AAFZ/xkJj+MDpKRXlk7luirTkdzkz9eUSWpXpU1HpssLP3TJlDIeRnwSn3m154zsqu4Z2HSlcpt6/8Y+Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e614148e40935ac5663308f5072be25bae1b0beadcc929ae485c5a46b675910f","last_reissued_at":"2026-05-18T01:21:26.124990Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:21:26.124990Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Monte-Carlo radiative transfer simulation of the circumstellar disk of the Herbig Ae star HD 144432","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Kreplin, D. Schertl, F. Malbet, F. Massi, G. Weigelt, K.-H. Hofmann, L. Chen, Ph. Stee, R. Petrov","submitted_at":"2015-12-07T22:48:16Z","abstract_excerpt":"Studies of pre-transitional disks, with a gap region between the inner infrared-emitting region and the outer disk, are important to improving our understanding of disk evolution and planet formation. Previous infrared interferometric observations have shown hints of a gap region in the protoplanetary disk around the Herbig Ae star HD~144432. We study the dust distribution around this star with two-dimensional radiative transfer modeling. We compare the model predictions obtained via the Monte-Carlo radiative transfer code RADMC-3D with infrared interferometric observations and the {\\SED} of H"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1512.02276","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":""},"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":"1512.02276","created_at":"2026-05-18T01:21:26.125082+00:00"},{"alias_kind":"arxiv_version","alias_value":"1512.02276v1","created_at":"2026-05-18T01:21:26.125082+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1512.02276","created_at":"2026-05-18T01:21:26.125082+00:00"},{"alias_kind":"pith_short_12","alias_value":"4YKBJDSASNNM","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_16","alias_value":"4YKBJDSASNNMKZRT","created_at":"2026-05-18T12:29:05.191682+00:00"},{"alias_kind":"pith_short_8","alias_value":"4YKBJDSA","created_at":"2026-05-18T12:29:05.191682+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/4YKBJDSASNNMKZRTBD2QOK7CLO","json":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO.json","graph_json":"https://pith.science/api/pith-number/4YKBJDSASNNMKZRTBD2QOK7CLO/graph.json","events_json":"https://pith.science/api/pith-number/4YKBJDSASNNMKZRTBD2QOK7CLO/events.json","paper":"https://pith.science/paper/4YKBJDSA"},"agent_actions":{"view_html":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO","download_json":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO.json","view_paper":"https://pith.science/paper/4YKBJDSA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1512.02276&json=true","fetch_graph":"https://pith.science/api/pith-number/4YKBJDSASNNMKZRTBD2QOK7CLO/graph.json","fetch_events":"https://pith.science/api/pith-number/4YKBJDSASNNMKZRTBD2QOK7CLO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO/action/storage_attestation","attest_author":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO/action/author_attestation","sign_citation":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO/action/citation_signature","submit_replication":"https://pith.science/pith/4YKBJDSASNNMKZRTBD2QOK7CLO/action/replication_record"}},"created_at":"2026-05-18T01:21:26.125082+00:00","updated_at":"2026-05-18T01:21:26.125082+00:00"}