{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2009:I4SAIF4LOT3YK3MLTPGBGBJOVR","short_pith_number":"pith:I4SAIF4L","canonical_record":{"source":{"id":"0905.2965","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-05-18T20:00:51Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"c4df590abb17fd7f3c667a5c04ebf06d41d4325e11fb7aa7a1ea6b7f2c026cd6","abstract_canon_sha256":"9897b60d80b5a3aa56885e63fd2c75a086a3cd4111d3473c925dfc0f5259c0ab"},"schema_version":"1.0"},"canonical_sha256":"472404178b74f7856d8b9bcc13052eac7ca48dfd3d1c7b9d834ee1859c6b40e5","source":{"kind":"arxiv","id":"0905.2965","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"0905.2965","created_at":"2026-05-18T02:13:38Z"},{"alias_kind":"arxiv_version","alias_value":"0905.2965v1","created_at":"2026-05-18T02:13:38Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0905.2965","created_at":"2026-05-18T02:13:38Z"},{"alias_kind":"pith_short_12","alias_value":"I4SAIF4LOT3Y","created_at":"2026-05-18T12:25:59Z"},{"alias_kind":"pith_short_16","alias_value":"I4SAIF4LOT3YK3ML","created_at":"2026-05-18T12:25:59Z"},{"alias_kind":"pith_short_8","alias_value":"I4SAIF4L","created_at":"2026-05-18T12:25:59Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2009:I4SAIF4LOT3YK3MLTPGBGBJOVR","target":"record","payload":{"canonical_record":{"source":{"id":"0905.2965","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-05-18T20:00:51Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"c4df590abb17fd7f3c667a5c04ebf06d41d4325e11fb7aa7a1ea6b7f2c026cd6","abstract_canon_sha256":"9897b60d80b5a3aa56885e63fd2c75a086a3cd4111d3473c925dfc0f5259c0ab"},"schema_version":"1.0"},"canonical_sha256":"472404178b74f7856d8b9bcc13052eac7ca48dfd3d1c7b9d834ee1859c6b40e5","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:13:38.812092Z","signature_b64":"H7DOAfD7Lt0QSpw09fike3o9hGr6UTV2emF4ARKL/6rK+jkBllUOpKjFUJRDq+t8qySaoXPhWNgYKjELbjfuDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"472404178b74f7856d8b9bcc13052eac7ca48dfd3d1c7b9d834ee1859c6b40e5","last_reissued_at":"2026-05-18T02:13:38.811515Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:13:38.811515Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"0905.2965","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":"2026-05-18T02:13:38Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"VgvBdouSmz6xAM1PMMawQ/5vanDYzmkFdU0ziYZqKSiqP6X5+HMSjIfyeZmSJpjeddzGNcenzFT2yvWNfrC9BA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T11:32:09.959771Z"},"content_sha256":"c9f495d6eb1121f2b125a779996179391ca64ecf5bea06205d37671541d62180","schema_version":"1.0","event_id":"sha256:c9f495d6eb1121f2b125a779996179391ca64ecf5bea06205d37671541d62180"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2009:I4SAIF4LOT3YK3MLTPGBGBJOVR","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"On the large-scale outflows in active galactic nuclei: consequences of coupling the mass-supply rate and accretion luminosity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Daniel Proga, Ryuichi Kurosawa","submitted_at":"2009-05-18T20:00:51Z","abstract_excerpt":"(Abridged) We present two-dimensional hydrodynamical simulations of slowly rotating gas that is under the influence of the gravity of a super massive black hole and is irradiated by a thin UV accretion disc and a spherical X-ray corona. We calculate the accretion luminosity of a system based on the accretion-rate which is assumed to be equal to the mass-supply rate at the radius of ~10^-2 pc. For the models with high temperature gas at large radii (~10 pc) and high luminosities, we find a strong correlation between the mass-outflow rate (Mdot_out) and the luminosity (L). The power law index (q"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0905.2965","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":"2026-05-18T02:13:38Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"tTgd2t3Ts4UxHeFamc6AK1jOnOOjzwYn3y+Gr6PTW2dNVxn43uRVmxcBty6jCwlo7s+u553cHI5ceMHmkUDQCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T11:32:09.960119Z"},"content_sha256":"ab11c861212127479d718674c88a9c36ec458f90c3c4610ab4c7ddbc9da6dcd3","schema_version":"1.0","event_id":"sha256:ab11c861212127479d718674c88a9c36ec458f90c3c4610ab4c7ddbc9da6dcd3"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/I4SAIF4LOT3YK3MLTPGBGBJOVR/bundle.json","state_url":"https://pith.science/pith/I4SAIF4LOT3YK3MLTPGBGBJOVR/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/I4SAIF4LOT3YK3MLTPGBGBJOVR/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":"2026-06-04T11:32:09Z","links":{"resolver":"https://pith.science/pith/I4SAIF4LOT3YK3MLTPGBGBJOVR","bundle":"https://pith.science/pith/I4SAIF4LOT3YK3MLTPGBGBJOVR/bundle.json","state":"https://pith.science/pith/I4SAIF4LOT3YK3MLTPGBGBJOVR/state.json","well_known_bundle":"https://pith.science/.well-known/pith/I4SAIF4LOT3YK3MLTPGBGBJOVR/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2009:I4SAIF4LOT3YK3MLTPGBGBJOVR","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":"9897b60d80b5a3aa56885e63fd2c75a086a3cd4111d3473c925dfc0f5259c0ab","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-05-18T20:00:51Z","title_canon_sha256":"c4df590abb17fd7f3c667a5c04ebf06d41d4325e11fb7aa7a1ea6b7f2c026cd6"},"schema_version":"1.0","source":{"id":"0905.2965","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"0905.2965","created_at":"2026-05-18T02:13:38Z"},{"alias_kind":"arxiv_version","alias_value":"0905.2965v1","created_at":"2026-05-18T02:13:38Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0905.2965","created_at":"2026-05-18T02:13:38Z"},{"alias_kind":"pith_short_12","alias_value":"I4SAIF4LOT3Y","created_at":"2026-05-18T12:25:59Z"},{"alias_kind":"pith_short_16","alias_value":"I4SAIF4LOT3YK3ML","created_at":"2026-05-18T12:25:59Z"},{"alias_kind":"pith_short_8","alias_value":"I4SAIF4L","created_at":"2026-05-18T12:25:59Z"}],"graph_snapshots":[{"event_id":"sha256:ab11c861212127479d718674c88a9c36ec458f90c3c4610ab4c7ddbc9da6dcd3","target":"graph","created_at":"2026-05-18T02:13:38Z","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":"(Abridged) We present two-dimensional hydrodynamical simulations of slowly rotating gas that is under the influence of the gravity of a super massive black hole and is irradiated by a thin UV accretion disc and a spherical X-ray corona. We calculate the accretion luminosity of a system based on the accretion-rate which is assumed to be equal to the mass-supply rate at the radius of ~10^-2 pc. For the models with high temperature gas at large radii (~10 pc) and high luminosities, we find a strong correlation between the mass-outflow rate (Mdot_out) and the luminosity (L). The power law index (q","authors_text":"Daniel Proga, Ryuichi Kurosawa","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-05-18T20:00:51Z","title":"On the large-scale outflows in active galactic nuclei: consequences of coupling the mass-supply rate and accretion luminosity"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0905.2965","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:c9f495d6eb1121f2b125a779996179391ca64ecf5bea06205d37671541d62180","target":"record","created_at":"2026-05-18T02:13:38Z","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":"9897b60d80b5a3aa56885e63fd2c75a086a3cd4111d3473c925dfc0f5259c0ab","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2009-05-18T20:00:51Z","title_canon_sha256":"c4df590abb17fd7f3c667a5c04ebf06d41d4325e11fb7aa7a1ea6b7f2c026cd6"},"schema_version":"1.0","source":{"id":"0905.2965","kind":"arxiv","version":1}},"canonical_sha256":"472404178b74f7856d8b9bcc13052eac7ca48dfd3d1c7b9d834ee1859c6b40e5","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"472404178b74f7856d8b9bcc13052eac7ca48dfd3d1c7b9d834ee1859c6b40e5","first_computed_at":"2026-05-18T02:13:38.811515Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:13:38.811515Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"H7DOAfD7Lt0QSpw09fike3o9hGr6UTV2emF4ARKL/6rK+jkBllUOpKjFUJRDq+t8qySaoXPhWNgYKjELbjfuDg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:13:38.812092Z","signed_message":"canonical_sha256_bytes"},"source_id":"0905.2965","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:c9f495d6eb1121f2b125a779996179391ca64ecf5bea06205d37671541d62180","sha256:ab11c861212127479d718674c88a9c36ec458f90c3c4610ab4c7ddbc9da6dcd3"],"state_sha256":"3fc8eac55cb1d1fc9e8c4968a307a38e8c652695b7bb13a03dfabd07e1499d4c"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"moCcwwbzGgI8IgRulfT8KmDjB521d+hp2VygINmaSPy1pQb6wO8BzvJ53JRQG09mzw+Hpoy3+99IC5PP1+wnAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T11:32:09.962101Z","bundle_sha256":"0889b7a936e6465a08e3e90c66130d7d850b1b8a3695585511a5349a03dbb6c3"}}