{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:PWALS3FVGWMOI73MTZLDIZ5F3H","short_pith_number":"pith:PWALS3FV","canonical_record":{"source":{"id":"1202.4681","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-02-21T15:52:51Z","cross_cats_sorted":[],"title_canon_sha256":"b8f9e7ab52593d887b2926213ef30afff1e4d456bcf611287b86973829f94b0d","abstract_canon_sha256":"70565f69fa7aa6ceb4e0af300db813b2f1e2024952d7fd7fa4f5cbd950f7ce49"},"schema_version":"1.0"},"canonical_sha256":"7d80b96cb53598e47f6c9e563467a5d9d1d77f74fd911f8ad0c3cb2580909bc1","source":{"kind":"arxiv","id":"1202.4681","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1202.4681","created_at":"2026-05-18T01:58:22Z"},{"alias_kind":"arxiv_version","alias_value":"1202.4681v1","created_at":"2026-05-18T01:58:22Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.4681","created_at":"2026-05-18T01:58:22Z"},{"alias_kind":"pith_short_12","alias_value":"PWALS3FVGWMO","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_16","alias_value":"PWALS3FVGWMOI73M","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_8","alias_value":"PWALS3FV","created_at":"2026-05-18T12:27:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:PWALS3FVGWMOI73MTZLDIZ5F3H","target":"record","payload":{"canonical_record":{"source":{"id":"1202.4681","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-02-21T15:52:51Z","cross_cats_sorted":[],"title_canon_sha256":"b8f9e7ab52593d887b2926213ef30afff1e4d456bcf611287b86973829f94b0d","abstract_canon_sha256":"70565f69fa7aa6ceb4e0af300db813b2f1e2024952d7fd7fa4f5cbd950f7ce49"},"schema_version":"1.0"},"canonical_sha256":"7d80b96cb53598e47f6c9e563467a5d9d1d77f74fd911f8ad0c3cb2580909bc1","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:22.829994Z","signature_b64":"Fi8GaOLrxXcT+zcVmsYzazrglaLE7QSlNkDClkMiTghtrgy6af/MZ5VZ2nR4SB+6qc7xC58elf7mrBN1+qwDAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7d80b96cb53598e47f6c9e563467a5d9d1d77f74fd911f8ad0c3cb2580909bc1","last_reissued_at":"2026-05-18T01:58:22.829476Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:22.829476Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1202.4681","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":"2026-05-18T01:58:22Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ZZQSHSCLMroa53qQev+M4/z3Z1N4aVc/GjVeCnrxoeLD7IyhHzeJK+Fmbo9/rA9rYsxADcLhh0K9O5sauSMwAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T23:44:58.371198Z"},"content_sha256":"42cd779742a30f077b1ec76e1bf069c71e487abf5ecc197f1d8865bbfa6f1d72","schema_version":"1.0","event_id":"sha256:42cd779742a30f077b1ec76e1bf069c71e487abf5ecc197f1d8865bbfa6f1d72"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:PWALS3FVGWMOI73MTZLDIZ5F3H","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Sweeping Away the Mysteries of Dusty Continuous Winds in AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"2), (2) University of Toronto, (3) University of Wisconsin), J. E. Everett (3), R. P. Deo (1) ((1) University of Western Ontario, S. C. Gallagher (1), S. K. Keating (1","submitted_at":"2012-02-21T15:52:51Z","abstract_excerpt":"An integral part of the Unified Model for Active Galactic Nuclei (AGNs) is an axisymmetric obscuring medium, which is commonly depicted as a torus of gas and dust surrounding the central engine. However, a robust, dynamical model of the torus is required in order to understand the fundamental physics of AGNs and interpret their observational signatures. Here we explore self-similar, dusty disk-winds, driven by both magnetocentrifugal forces and radiation pressure, as an explanation for the torus. Using these models, we make predictions of AGN infrared (IR) spectral energy distributions (SEDs) "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.4681","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":"2026-05-18T01:58:22Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"j3QeCbpcVx75itCeBifEtlhOUbnXhcKWwfYo7coN7ZTqnUTck15TLhfAtWAnyk3ICqT1p/Z5SImmtyDv0RdzDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T23:44:58.371886Z"},"content_sha256":"978b9b5c20d645e9f7884199f2b0e552fc2857062dfc9436e9a28cee72fc12c6","schema_version":"1.0","event_id":"sha256:978b9b5c20d645e9f7884199f2b0e552fc2857062dfc9436e9a28cee72fc12c6"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PWALS3FVGWMOI73MTZLDIZ5F3H/bundle.json","state_url":"https://pith.science/pith/PWALS3FVGWMOI73MTZLDIZ5F3H/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PWALS3FVGWMOI73MTZLDIZ5F3H/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":"2026-06-06T23:44:58Z","links":{"resolver":"https://pith.science/pith/PWALS3FVGWMOI73MTZLDIZ5F3H","bundle":"https://pith.science/pith/PWALS3FVGWMOI73MTZLDIZ5F3H/bundle.json","state":"https://pith.science/pith/PWALS3FVGWMOI73MTZLDIZ5F3H/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PWALS3FVGWMOI73MTZLDIZ5F3H/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:PWALS3FVGWMOI73MTZLDIZ5F3H","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":"70565f69fa7aa6ceb4e0af300db813b2f1e2024952d7fd7fa4f5cbd950f7ce49","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-02-21T15:52:51Z","title_canon_sha256":"b8f9e7ab52593d887b2926213ef30afff1e4d456bcf611287b86973829f94b0d"},"schema_version":"1.0","source":{"id":"1202.4681","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1202.4681","created_at":"2026-05-18T01:58:22Z"},{"alias_kind":"arxiv_version","alias_value":"1202.4681v1","created_at":"2026-05-18T01:58:22Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.4681","created_at":"2026-05-18T01:58:22Z"},{"alias_kind":"pith_short_12","alias_value":"PWALS3FVGWMO","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_16","alias_value":"PWALS3FVGWMOI73M","created_at":"2026-05-18T12:27:18Z"},{"alias_kind":"pith_short_8","alias_value":"PWALS3FV","created_at":"2026-05-18T12:27:18Z"}],"graph_snapshots":[{"event_id":"sha256:978b9b5c20d645e9f7884199f2b0e552fc2857062dfc9436e9a28cee72fc12c6","target":"graph","created_at":"2026-05-18T01:58:22Z","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":"An integral part of the Unified Model for Active Galactic Nuclei (AGNs) is an axisymmetric obscuring medium, which is commonly depicted as a torus of gas and dust surrounding the central engine. However, a robust, dynamical model of the torus is required in order to understand the fundamental physics of AGNs and interpret their observational signatures. Here we explore self-similar, dusty disk-winds, driven by both magnetocentrifugal forces and radiation pressure, as an explanation for the torus. Using these models, we make predictions of AGN infrared (IR) spectral energy distributions (SEDs) ","authors_text":"2), (2) University of Toronto, (3) University of Wisconsin), J. E. Everett (3), R. P. Deo (1) ((1) University of Western Ontario, S. C. Gallagher (1), S. K. Keating (1","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-02-21T15:52:51Z","title":"Sweeping Away the Mysteries of Dusty Continuous Winds in AGN"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.4681","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":"sha256:42cd779742a30f077b1ec76e1bf069c71e487abf5ecc197f1d8865bbfa6f1d72","target":"record","created_at":"2026-05-18T01:58:22Z","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":"70565f69fa7aa6ceb4e0af300db813b2f1e2024952d7fd7fa4f5cbd950f7ce49","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-02-21T15:52:51Z","title_canon_sha256":"b8f9e7ab52593d887b2926213ef30afff1e4d456bcf611287b86973829f94b0d"},"schema_version":"1.0","source":{"id":"1202.4681","kind":"arxiv","version":1}},"canonical_sha256":"7d80b96cb53598e47f6c9e563467a5d9d1d77f74fd911f8ad0c3cb2580909bc1","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"7d80b96cb53598e47f6c9e563467a5d9d1d77f74fd911f8ad0c3cb2580909bc1","first_computed_at":"2026-05-18T01:58:22.829476Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:58:22.829476Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Fi8GaOLrxXcT+zcVmsYzazrglaLE7QSlNkDClkMiTghtrgy6af/MZ5VZ2nR4SB+6qc7xC58elf7mrBN1+qwDAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:58:22.829994Z","signed_message":"canonical_sha256_bytes"},"source_id":"1202.4681","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:42cd779742a30f077b1ec76e1bf069c71e487abf5ecc197f1d8865bbfa6f1d72","sha256:978b9b5c20d645e9f7884199f2b0e552fc2857062dfc9436e9a28cee72fc12c6"],"state_sha256":"dc24a87055beff0480d64b8be581d21cbc0b9d6bfbf0232a3f508a0e93334a0e"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"JZQ8eyFWGjrHroDDiSAzLGO1LIR4Rqs4TntOMH8rt3oJCwIpZpm0SS4kSIaVtALEhKANxwXMQVrJfR8Xm1+rDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-06T23:44:58.375592Z","bundle_sha256":"bf98c1b8a9209f8ef2da5cc66db9290bd02c22932286326adfede046ea034129"}}