{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:GSMV7STXNNBIXCAPMLUWIXKXEC","short_pith_number":"pith:GSMV7STX","canonical_record":{"source":{"id":"1706.07958","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-24T13:49:43Z","cross_cats_sorted":[],"title_canon_sha256":"7be975571daa6f823461334768bbf4c14d0a7659ede2903065d66bda6d05edbe","abstract_canon_sha256":"27aec6ec77f3ddca3e4e9dc6a2dd81ebca529899b3acaa0e2c6af8690e4f1ba1"},"schema_version":"1.0"},"canonical_sha256":"34995fca776b428b880f62e9645d57208e7f439459f5e825a246041d9eb68076","source":{"kind":"arxiv","id":"1706.07958","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.07958","created_at":"2026-05-18T00:34:47Z"},{"alias_kind":"arxiv_version","alias_value":"1706.07958v2","created_at":"2026-05-18T00:34:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.07958","created_at":"2026-05-18T00:34:47Z"},{"alias_kind":"pith_short_12","alias_value":"GSMV7STXNNBI","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"GSMV7STXNNBIXCAP","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"GSMV7STX","created_at":"2026-05-18T12:31:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:GSMV7STXNNBIXCAPMLUWIXKXEC","target":"record","payload":{"canonical_record":{"source":{"id":"1706.07958","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-24T13:49:43Z","cross_cats_sorted":[],"title_canon_sha256":"7be975571daa6f823461334768bbf4c14d0a7659ede2903065d66bda6d05edbe","abstract_canon_sha256":"27aec6ec77f3ddca3e4e9dc6a2dd81ebca529899b3acaa0e2c6af8690e4f1ba1"},"schema_version":"1.0"},"canonical_sha256":"34995fca776b428b880f62e9645d57208e7f439459f5e825a246041d9eb68076","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:34:47.635516Z","signature_b64":"UplMWh1RMwNFouLh6UxzRp2w6FR3RD1FCH9D+CEMA1pIGHP7mCMS7gmjPZzC/08pTik53DwLby7yQn4s8navAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"34995fca776b428b880f62e9645d57208e7f439459f5e825a246041d9eb68076","last_reissued_at":"2026-05-18T00:34:47.634774Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:34:47.634774Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1706.07958","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:34:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"wN1kQe459nMVVzr8LccYqhVfQvjkDiP7VW3oD9ZHsNyV7eA30WyI67EjPxJ3FAXQjg32JqCJbBb9SsXALBIMCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T16:23:44.202699Z"},"content_sha256":"dce2155d397712b9db940a5b153bf5a9df5ca4dff4734956370e6ecd72cb7d1d","schema_version":"1.0","event_id":"sha256:dce2155d397712b9db940a5b153bf5a9df5ca4dff4734956370e6ecd72cb7d1d"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:GSMV7STXNNBIXCAPMLUWIXKXEC","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Failed radiatively Accelerated Dusty Outflow model of the Broad Line Region in Active Galactic Nuclei. I. Analytical solution","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. Czerny, C. Wildy, J.-M. Wang, J. Sredzinska, K. Hryniewicz, M. Sniegowska, S. Panda, V. Karas, Yan-Rong Li","submitted_at":"2017-06-24T13:49:43Z","abstract_excerpt":"The physical origin of the Broad Line Region in Active Galactic Nuclei is still unclear despite many years of observational studies. The reason is that the region is unresolved and the reverberation mapping results imply complex velocity field. We adopt a theory-motivated approach to identify the principal mechanism responsible for this complex phenomenon. We consider the possibility that the role of dust is essential. We assume that the local radiation pressure acting on the dust in the accretion disk atmosphere launches the outflow of material, but higher above the disk the irradiation from "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.07958","kind":"arxiv","version":2},"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":"2026-05-18T00:34:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"uK0Oc6pJZ1M12tcrTWsj9d9TwLSwFTrMHgu3e3wMldcdpvcGgMogkT86918O9AgO9QkSNxpDLOy6EIJ1iH1sDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T16:23:44.203053Z"},"content_sha256":"b9b43ebafb71df3c0dfd747324bbebe48731597c33406e828df0a4661dbce809","schema_version":"1.0","event_id":"sha256:b9b43ebafb71df3c0dfd747324bbebe48731597c33406e828df0a4661dbce809"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GSMV7STXNNBIXCAPMLUWIXKXEC/bundle.json","state_url":"https://pith.science/pith/GSMV7STXNNBIXCAPMLUWIXKXEC/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GSMV7STXNNBIXCAPMLUWIXKXEC/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":"2026-05-19T16:23:44Z","links":{"resolver":"https://pith.science/pith/GSMV7STXNNBIXCAPMLUWIXKXEC","bundle":"https://pith.science/pith/GSMV7STXNNBIXCAPMLUWIXKXEC/bundle.json","state":"https://pith.science/pith/GSMV7STXNNBIXCAPMLUWIXKXEC/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GSMV7STXNNBIXCAPMLUWIXKXEC/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:GSMV7STXNNBIXCAPMLUWIXKXEC","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":"27aec6ec77f3ddca3e4e9dc6a2dd81ebca529899b3acaa0e2c6af8690e4f1ba1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-24T13:49:43Z","title_canon_sha256":"7be975571daa6f823461334768bbf4c14d0a7659ede2903065d66bda6d05edbe"},"schema_version":"1.0","source":{"id":"1706.07958","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.07958","created_at":"2026-05-18T00:34:47Z"},{"alias_kind":"arxiv_version","alias_value":"1706.07958v2","created_at":"2026-05-18T00:34:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.07958","created_at":"2026-05-18T00:34:47Z"},{"alias_kind":"pith_short_12","alias_value":"GSMV7STXNNBI","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"GSMV7STXNNBIXCAP","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"GSMV7STX","created_at":"2026-05-18T12:31:18Z"}],"graph_snapshots":[{"event_id":"sha256:b9b43ebafb71df3c0dfd747324bbebe48731597c33406e828df0a4661dbce809","target":"graph","created_at":"2026-05-18T00:34:47Z","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":"The physical origin of the Broad Line Region in Active Galactic Nuclei is still unclear despite many years of observational studies. The reason is that the region is unresolved and the reverberation mapping results imply complex velocity field. We adopt a theory-motivated approach to identify the principal mechanism responsible for this complex phenomenon. We consider the possibility that the role of dust is essential. We assume that the local radiation pressure acting on the dust in the accretion disk atmosphere launches the outflow of material, but higher above the disk the irradiation from ","authors_text":"B. Czerny, C. Wildy, J.-M. Wang, J. Sredzinska, K. Hryniewicz, M. Sniegowska, S. Panda, V. Karas, Yan-Rong Li","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-24T13:49:43Z","title":"Failed radiatively Accelerated Dusty Outflow model of the Broad Line Region in Active Galactic Nuclei. I. Analytical solution"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.07958","kind":"arxiv","version":2},"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:dce2155d397712b9db940a5b153bf5a9df5ca4dff4734956370e6ecd72cb7d1d","target":"record","created_at":"2026-05-18T00:34:47Z","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":"27aec6ec77f3ddca3e4e9dc6a2dd81ebca529899b3acaa0e2c6af8690e4f1ba1","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-24T13:49:43Z","title_canon_sha256":"7be975571daa6f823461334768bbf4c14d0a7659ede2903065d66bda6d05edbe"},"schema_version":"1.0","source":{"id":"1706.07958","kind":"arxiv","version":2}},"canonical_sha256":"34995fca776b428b880f62e9645d57208e7f439459f5e825a246041d9eb68076","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"34995fca776b428b880f62e9645d57208e7f439459f5e825a246041d9eb68076","first_computed_at":"2026-05-18T00:34:47.634774Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:34:47.634774Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"UplMWh1RMwNFouLh6UxzRp2w6FR3RD1FCH9D+CEMA1pIGHP7mCMS7gmjPZzC/08pTik53DwLby7yQn4s8navAg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:34:47.635516Z","signed_message":"canonical_sha256_bytes"},"source_id":"1706.07958","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:dce2155d397712b9db940a5b153bf5a9df5ca4dff4734956370e6ecd72cb7d1d","sha256:b9b43ebafb71df3c0dfd747324bbebe48731597c33406e828df0a4661dbce809"],"state_sha256":"dee0ac932bb52f5b6df6eff02eee8ad9c0ff664faa8b90f42b95a443c24b03c4"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"b2m3LET34bsm6zIZFvp/+dpRlTJmP435T6lSsghTMfG3ye15CU2FFxWB+yO1bJlkoVSLMCUE7dHHt7EaiE1jBA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-19T16:23:44.205186Z","bundle_sha256":"e4c9f7d3299d29dbc655a3061d6b569eb95e762017a4f6c7f6c7ed9a824aa5ed"}}