{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:4FGQOFAXVKBQGMR3PNN3ZDGMMH","short_pith_number":"pith:4FGQOFAX","schema_version":"1.0","canonical_sha256":"e14d071417aa8303323b7b5bbc8ccc61fa5409ab32474f16342f179bca21dfd9","source":{"kind":"arxiv","id":"2308.05924","version":1},"attestation_state":"computed","paper":{"title":"Origin of the complex iron line structure and spectral variation in Mrk 766","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Ken Ebisawa, Misaki Mizumoto, Yuto Mochizuki","submitted_at":"2023-08-11T03:43:17Z","abstract_excerpt":"Complex Fe-K emission/absorption line features are commonly observed in the 6--11 keV band from Active Galactic Nuclei (AGN). These features are formed in various physical components surrounding the black holes. The Narrow-Line Seyfert 1 (NLS1) galaxy Mrk 766, in particular, exhibits characteristic blue-shifted Fe-K absorption lines caused by the ultra-fast outflow (UFO), and a broad Fe-K emission line, as well as variable absorbers partially covering the X-ray emitting region. We re-analyze the Mrk 766 archival data of XMM-Newton, NuSTAR, and Swift to investigate the origin of the Fe-K line f"},"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":"2308.05924","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-08-11T03:43:17Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"6c582b8c1555d61c3c615925fb657f2bae69c82a97fa18ab68846b0654c13c23","abstract_canon_sha256":"885a884a2d70a6662a40bb6f5f4b396b52f9c885ee9ccc9d8b5513e2384f6d2b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:40:20.726875Z","signature_b64":"2IkPQF5KNOWTSXeV4vD9Nj3zmWlqH9V++x0jLsVG/tXHi+pIL8mKekNOUN7BKYs6vXt7wYxSJztcY5rqDpxnAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e14d071417aa8303323b7b5bbc8ccc61fa5409ab32474f16342f179bca21dfd9","last_reissued_at":"2026-07-05T06:40:20.726400Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:40:20.726400Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Origin of the complex iron line structure and spectral variation in Mrk 766","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Ken Ebisawa, Misaki Mizumoto, Yuto Mochizuki","submitted_at":"2023-08-11T03:43:17Z","abstract_excerpt":"Complex Fe-K emission/absorption line features are commonly observed in the 6--11 keV band from Active Galactic Nuclei (AGN). These features are formed in various physical components surrounding the black holes. The Narrow-Line Seyfert 1 (NLS1) galaxy Mrk 766, in particular, exhibits characteristic blue-shifted Fe-K absorption lines caused by the ultra-fast outflow (UFO), and a broad Fe-K emission line, as well as variable absorbers partially covering the X-ray emitting region. We re-analyze the Mrk 766 archival data of XMM-Newton, NuSTAR, and Swift to investigate the origin of the Fe-K line f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.05924","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/2308.05924/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":"2308.05924","created_at":"2026-07-05T06:40:20.726454+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.05924v1","created_at":"2026-07-05T06:40:20.726454+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.05924","created_at":"2026-07-05T06:40:20.726454+00:00"},{"alias_kind":"pith_short_12","alias_value":"4FGQOFAXVKBQ","created_at":"2026-07-05T06:40:20.726454+00:00"},{"alias_kind":"pith_short_16","alias_value":"4FGQOFAXVKBQGMR3","created_at":"2026-07-05T06:40:20.726454+00:00"},{"alias_kind":"pith_short_8","alias_value":"4FGQOFAX","created_at":"2026-07-05T06:40:20.726454+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/4FGQOFAXVKBQGMR3PNN3ZDGMMH","json":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH.json","graph_json":"https://pith.science/api/pith-number/4FGQOFAXVKBQGMR3PNN3ZDGMMH/graph.json","events_json":"https://pith.science/api/pith-number/4FGQOFAXVKBQGMR3PNN3ZDGMMH/events.json","paper":"https://pith.science/paper/4FGQOFAX"},"agent_actions":{"view_html":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH","download_json":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH.json","view_paper":"https://pith.science/paper/4FGQOFAX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.05924&json=true","fetch_graph":"https://pith.science/api/pith-number/4FGQOFAXVKBQGMR3PNN3ZDGMMH/graph.json","fetch_events":"https://pith.science/api/pith-number/4FGQOFAXVKBQGMR3PNN3ZDGMMH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH/action/storage_attestation","attest_author":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH/action/author_attestation","sign_citation":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH/action/citation_signature","submit_replication":"https://pith.science/pith/4FGQOFAXVKBQGMR3PNN3ZDGMMH/action/replication_record"}},"created_at":"2026-07-05T06:40:20.726454+00:00","updated_at":"2026-07-05T06:40:20.726454+00:00"}