{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:ZW633BGYG47QIMZSWFMFC5J565","short_pith_number":"pith:ZW633BGY","canonical_record":{"source":{"id":"1204.2535","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-04-11T19:52:17Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"25971fa455d12e681ff7d0c7ce7360f0a9be7971e69e717e99146f64ed25a89e","abstract_canon_sha256":"ba6dd0249d2697890dd2a56f1b4f5822d699fc96e64f8377ccd983f11467c4b0"},"schema_version":"1.0"},"canonical_sha256":"cdbdbd84d8373f043332b15851753df7542eb1d7aa0ca4a077078f6e7cc81654","source":{"kind":"arxiv","id":"1204.2535","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1204.2535","created_at":"2026-05-18T03:54:37Z"},{"alias_kind":"arxiv_version","alias_value":"1204.2535v1","created_at":"2026-05-18T03:54:37Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.2535","created_at":"2026-05-18T03:54:37Z"},{"alias_kind":"pith_short_12","alias_value":"ZW633BGYG47Q","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_16","alias_value":"ZW633BGYG47QIMZS","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_8","alias_value":"ZW633BGY","created_at":"2026-05-18T12:27:30Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:ZW633BGYG47QIMZSWFMFC5J565","target":"record","payload":{"canonical_record":{"source":{"id":"1204.2535","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-04-11T19:52:17Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"25971fa455d12e681ff7d0c7ce7360f0a9be7971e69e717e99146f64ed25a89e","abstract_canon_sha256":"ba6dd0249d2697890dd2a56f1b4f5822d699fc96e64f8377ccd983f11467c4b0"},"schema_version":"1.0"},"canonical_sha256":"cdbdbd84d8373f043332b15851753df7542eb1d7aa0ca4a077078f6e7cc81654","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:54:37.028421Z","signature_b64":"NspTtnmFfIGS1EGTtbhtq8daev8+QYdAGwUx82oWgP7MxZfNCoWNzQZSui8vrBlrXG0h4Yd+VFyAWDaOYlTJCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cdbdbd84d8373f043332b15851753df7542eb1d7aa0ca4a077078f6e7cc81654","last_reissued_at":"2026-05-18T03:54:37.027888Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:54:37.027888Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1204.2535","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:54:37Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"jV/dd4ITlwiaKoQGgK+Xer43GWw9B0BiiumeNQq8XKdhUAwA7onZA04TWZcMVgF85eETbWjlPygflo4cACdyCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T08:51:59.687597Z"},"content_sha256":"616d8f296dea51d728feb55331fa6fa38063d420b342f70cd699f34a736c6ca6","schema_version":"1.0","event_id":"sha256:616d8f296dea51d728feb55331fa6fa38063d420b342f70cd699f34a736c6ca6"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:ZW633BGYG47QIMZSWFMFC5J565","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Modeling the Fe K Line Profiles in Type I AGN with a Compton-Thick Disk Wind","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"A. R. Patrick, J. N. Reeves, K. S. Long, L. Miller, M. M. Tatum, S. A. Sim, T. J. Turner","submitted_at":"2012-04-11T19:52:17Z","abstract_excerpt":"We have modeled a small sample of Seyfert galaxies that were previously identified as having simple X-ray spectra with little intrinsic absorption. The sources in this sample all contain moderately broad components of Fe K-shell emission and are ideal candidates for testing the applicability of a Compton-thick accretion-disk wind model to AGN emission components. Viewing angles through the wind allow the observer to see the absorption signature of the gas, whereas face-on viewing angles allow the observer to see the scattered light from the wind. We find that the Fe K emission line profiles ar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.2535","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:54:37Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"sgGJ7EjwdLCiwCk9SNfQ+rD746v/m+2G2xrUyJt75HZypC2rz+E3MSnW362KAMEe56DTsjS1cBilkH6enBezAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T08:51:59.688335Z"},"content_sha256":"c822b08f40335ca1afe21fe8079cfd3e68ce8a805620b3de8712b23a17e852c6","schema_version":"1.0","event_id":"sha256:c822b08f40335ca1afe21fe8079cfd3e68ce8a805620b3de8712b23a17e852c6"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ZW633BGYG47QIMZSWFMFC5J565/bundle.json","state_url":"https://pith.science/pith/ZW633BGYG47QIMZSWFMFC5J565/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ZW633BGYG47QIMZSWFMFC5J565/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-27T08:51:59Z","links":{"resolver":"https://pith.science/pith/ZW633BGYG47QIMZSWFMFC5J565","bundle":"https://pith.science/pith/ZW633BGYG47QIMZSWFMFC5J565/bundle.json","state":"https://pith.science/pith/ZW633BGYG47QIMZSWFMFC5J565/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ZW633BGYG47QIMZSWFMFC5J565/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:ZW633BGYG47QIMZSWFMFC5J565","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"ba6dd0249d2697890dd2a56f1b4f5822d699fc96e64f8377ccd983f11467c4b0","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-04-11T19:52:17Z","title_canon_sha256":"25971fa455d12e681ff7d0c7ce7360f0a9be7971e69e717e99146f64ed25a89e"},"schema_version":"1.0","source":{"id":"1204.2535","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1204.2535","created_at":"2026-05-18T03:54:37Z"},{"alias_kind":"arxiv_version","alias_value":"1204.2535v1","created_at":"2026-05-18T03:54:37Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1204.2535","created_at":"2026-05-18T03:54:37Z"},{"alias_kind":"pith_short_12","alias_value":"ZW633BGYG47Q","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_16","alias_value":"ZW633BGYG47QIMZS","created_at":"2026-05-18T12:27:30Z"},{"alias_kind":"pith_short_8","alias_value":"ZW633BGY","created_at":"2026-05-18T12:27:30Z"}],"graph_snapshots":[{"event_id":"sha256:c822b08f40335ca1afe21fe8079cfd3e68ce8a805620b3de8712b23a17e852c6","target":"graph","created_at":"2026-05-18T03:54:37Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We have modeled a small sample of Seyfert galaxies that were previously identified as having simple X-ray spectra with little intrinsic absorption. The sources in this sample all contain moderately broad components of Fe K-shell emission and are ideal candidates for testing the applicability of a Compton-thick accretion-disk wind model to AGN emission components. Viewing angles through the wind allow the observer to see the absorption signature of the gas, whereas face-on viewing angles allow the observer to see the scattered light from the wind. We find that the Fe K emission line profiles ar","authors_text":"A. R. Patrick, J. N. Reeves, K. S. Long, L. Miller, M. M. Tatum, S. A. Sim, T. J. Turner","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-04-11T19:52:17Z","title":"Modeling the Fe K Line Profiles in Type I AGN with a Compton-Thick Disk Wind"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1204.2535","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:616d8f296dea51d728feb55331fa6fa38063d420b342f70cd699f34a736c6ca6","target":"record","created_at":"2026-05-18T03:54:37Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"ba6dd0249d2697890dd2a56f1b4f5822d699fc96e64f8377ccd983f11467c4b0","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-04-11T19:52:17Z","title_canon_sha256":"25971fa455d12e681ff7d0c7ce7360f0a9be7971e69e717e99146f64ed25a89e"},"schema_version":"1.0","source":{"id":"1204.2535","kind":"arxiv","version":1}},"canonical_sha256":"cdbdbd84d8373f043332b15851753df7542eb1d7aa0ca4a077078f6e7cc81654","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"cdbdbd84d8373f043332b15851753df7542eb1d7aa0ca4a077078f6e7cc81654","first_computed_at":"2026-05-18T03:54:37.027888Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:54:37.027888Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"NspTtnmFfIGS1EGTtbhtq8daev8+QYdAGwUx82oWgP7MxZfNCoWNzQZSui8vrBlrXG0h4Yd+VFyAWDaOYlTJCQ==","signature_status":"signed_v1","signed_at":"2026-05-18T03:54:37.028421Z","signed_message":"canonical_sha256_bytes"},"source_id":"1204.2535","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:616d8f296dea51d728feb55331fa6fa38063d420b342f70cd699f34a736c6ca6","sha256:c822b08f40335ca1afe21fe8079cfd3e68ce8a805620b3de8712b23a17e852c6"],"state_sha256":"1b508c1023e81769ea8f422a63d8782fc6b1734975d440b9878a3592b10b3292"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"0PWPsPM4bCyUAeZZMeg6h/ptd/85qGylnreW+DIIjxtgX2JfgmC39bFysf0AECV6nPoghnvIXTzRtSwKLdl5CA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T08:51:59.692236Z","bundle_sha256":"9003c107e77c9f97ae8c245543a84f47103e9c691fa2a78cda8c12d2b572e082"}}