{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:BQBDKTMXADEIQJKB37UUUXL24W","short_pith_number":"pith:BQBDKTMX","schema_version":"1.0","canonical_sha256":"0c02354d9700c8882541dfe94a5d7ae59ec305538c884a892fa1a7bcaffbe9d2","source":{"kind":"arxiv","id":"1602.00806","version":1},"attestation_state":"computed","paper":{"title":"X-ray Spectral Model of Reprocessing by Smooth and Clumpy Molecular Tori in Active Galactic Nuclei with the MONACO framework","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Hirokazu Odaka, Kazuma Hayashi, Masanori Ohno, Shun'ya Furui, Toshihiro Kawaguchi, Yasushi Fukazawa","submitted_at":"2016-02-02T07:00:43Z","abstract_excerpt":"We construct an X-ray spectral model of reprocessing by a torus in an active galactic nucleus (AGN) with a Monte Carlo simulation framework MONACO. Two torus geometries of smooth and clumpy cases are considered and compared. In order to reproduce a Compton shoulder accurately, MONACO includes not only free electron scattering but also bound electron scattering. Raman and Reyleigh scattering are also treated, and scattering cross sections dependent on chemical states of hydrogen and helium are included. Doppler broadening by turbulence velocity can be implemented. Our model gives consistent res"},"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":"1602.00806","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-02-02T07:00:43Z","cross_cats_sorted":[],"title_canon_sha256":"17adead8a788da76c5b93ed86add0b930dde6587256519d13e36d604b5a84bfc","abstract_canon_sha256":"d3783f3357baa3fd353a0cab6ccd34547a77dfff19305947c168ed30a6a57b26"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:19:24.543439Z","signature_b64":"sLVl26FpUVJMClCJxQOyB7I9nrZJoEh5rIV0iprg1NpGqsfwQQ037C00CygpK3vctmi3z1vjqARc4fKaFVZnAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0c02354d9700c8882541dfe94a5d7ae59ec305538c884a892fa1a7bcaffbe9d2","last_reissued_at":"2026-05-18T01:19:24.542747Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:19:24.542747Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray Spectral Model of Reprocessing by Smooth and Clumpy Molecular Tori in Active Galactic Nuclei with the MONACO framework","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Hirokazu Odaka, Kazuma Hayashi, Masanori Ohno, Shun'ya Furui, Toshihiro Kawaguchi, Yasushi Fukazawa","submitted_at":"2016-02-02T07:00:43Z","abstract_excerpt":"We construct an X-ray spectral model of reprocessing by a torus in an active galactic nucleus (AGN) with a Monte Carlo simulation framework MONACO. Two torus geometries of smooth and clumpy cases are considered and compared. In order to reproduce a Compton shoulder accurately, MONACO includes not only free electron scattering but also bound electron scattering. Raman and Reyleigh scattering are also treated, and scattering cross sections dependent on chemical states of hydrogen and helium are included. Doppler broadening by turbulence velocity can be implemented. Our model gives consistent res"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.00806","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":"1602.00806","created_at":"2026-05-18T01:19:24.542865+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.00806v1","created_at":"2026-05-18T01:19:24.542865+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.00806","created_at":"2026-05-18T01:19:24.542865+00:00"},{"alias_kind":"pith_short_12","alias_value":"BQBDKTMXADEI","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_16","alias_value":"BQBDKTMXADEIQJKB","created_at":"2026-05-18T12:30:07.202191+00:00"},{"alias_kind":"pith_short_8","alias_value":"BQBDKTMX","created_at":"2026-05-18T12:30:07.202191+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/BQBDKTMXADEIQJKB37UUUXL24W","json":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W.json","graph_json":"https://pith.science/api/pith-number/BQBDKTMXADEIQJKB37UUUXL24W/graph.json","events_json":"https://pith.science/api/pith-number/BQBDKTMXADEIQJKB37UUUXL24W/events.json","paper":"https://pith.science/paper/BQBDKTMX"},"agent_actions":{"view_html":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W","download_json":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W.json","view_paper":"https://pith.science/paper/BQBDKTMX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.00806&json=true","fetch_graph":"https://pith.science/api/pith-number/BQBDKTMXADEIQJKB37UUUXL24W/graph.json","fetch_events":"https://pith.science/api/pith-number/BQBDKTMXADEIQJKB37UUUXL24W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W/action/storage_attestation","attest_author":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W/action/author_attestation","sign_citation":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W/action/citation_signature","submit_replication":"https://pith.science/pith/BQBDKTMXADEIQJKB37UUUXL24W/action/replication_record"}},"created_at":"2026-05-18T01:19:24.542865+00:00","updated_at":"2026-05-18T01:19:24.542865+00:00"}