{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:YNNCXTBJ76FYQND7XMCI35V4LJ","short_pith_number":"pith:YNNCXTBJ","canonical_record":{"source":{"id":"1301.1147","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-07T10:29:59Z","cross_cats_sorted":[],"title_canon_sha256":"4a586b146ebee6c7e03a28d11bec4687e85c001d4fce87ba9bfd67778c83fa1c","abstract_canon_sha256":"06759393cf8c969ac1725427504173ab94135519f94cd904e219e781ddb7adc9"},"schema_version":"1.0"},"canonical_sha256":"c35a2bcc29ff8b88347fbb048df6bc5a7d0f0c4311ee24d10a3c0a499d5c1e4c","source":{"kind":"arxiv","id":"1301.1147","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1301.1147","created_at":"2026-05-18T01:52:21Z"},{"alias_kind":"arxiv_version","alias_value":"1301.1147v2","created_at":"2026-05-18T01:52:21Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.1147","created_at":"2026-05-18T01:52:21Z"},{"alias_kind":"pith_short_12","alias_value":"YNNCXTBJ76FY","created_at":"2026-05-18T12:28:06Z"},{"alias_kind":"pith_short_16","alias_value":"YNNCXTBJ76FYQND7","created_at":"2026-05-18T12:28:06Z"},{"alias_kind":"pith_short_8","alias_value":"YNNCXTBJ","created_at":"2026-05-18T12:28:06Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:YNNCXTBJ76FYQND7XMCI35V4LJ","target":"record","payload":{"canonical_record":{"source":{"id":"1301.1147","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-07T10:29:59Z","cross_cats_sorted":[],"title_canon_sha256":"4a586b146ebee6c7e03a28d11bec4687e85c001d4fce87ba9bfd67778c83fa1c","abstract_canon_sha256":"06759393cf8c969ac1725427504173ab94135519f94cd904e219e781ddb7adc9"},"schema_version":"1.0"},"canonical_sha256":"c35a2bcc29ff8b88347fbb048df6bc5a7d0f0c4311ee24d10a3c0a499d5c1e4c","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:52:21.142912Z","signature_b64":"KgQIHXWFYiVcPGwKQFreZAxOh2valtiEVVrWhJDQZG5MpniwWvwKbXGueuSIKOO/oNiNz28F8lK5bMrQ4l/JAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c35a2bcc29ff8b88347fbb048df6bc5a7d0f0c4311ee24d10a3c0a499d5c1e4c","last_reissued_at":"2026-05-18T01:52:21.142505Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:52:21.142505Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1301.1147","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":"2026-05-18T01:52:21Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"9ULU8WAyIXGOPDXoODevmqUWkHgYCGmVDM3+2BC5tmzMqKvQvIMgQRcNqtjMhc2xjheNq3Y7B66wSmIvg9RtAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T11:13:44.158633Z"},"content_sha256":"d2698307e8d45d39df20146bbe5090f9340e0f8c03278136f41e7c41e7c83564","schema_version":"1.0","event_id":"sha256:d2698307e8d45d39df20146bbe5090f9340e0f8c03278136f41e7c41e7c83564"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:YNNCXTBJ76FYQND7XMCI35V4LJ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Flux Modulation from the Rossby Wave Instability in microquasars accretion disks: toward a HFQPO model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"F. H. Vincent, H. Meheut, P. Varniere, T. Paumard","submitted_at":"2013-01-07T10:29:59Z","abstract_excerpt":"Context. There have been a long string of efforts to understand the source of the variability observed in microquasars, especially concerning the elusive High-Frequency Quasi-Periodic Oscillation. These oscillations are among the fastest phenomena that affect matter in the vicinity of stellar black holes and therefore could be used as probes of strong-field general relativity. Nevertheless, no model has yet gained wide acceptance. Aims. The aim of this article is to investigate the model derived from the occurrence of the Rossby wave instability at the inner edge of the accretion disk. In part"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.1147","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":"2026-05-18T01:52:21Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EOfIoPJnzPKbqscZzRa36vaRRD2tpKa8zonkhrKIt24I6hYoOi46PCs2FIc4X79ZymUSS6suwBTmvSr6T1bfBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-11T11:13:44.158980Z"},"content_sha256":"4c7078317c7d05eccf85aa6f9355bee5fd896fc20866f24bfa25e5864385ef1a","schema_version":"1.0","event_id":"sha256:4c7078317c7d05eccf85aa6f9355bee5fd896fc20866f24bfa25e5864385ef1a"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/YNNCXTBJ76FYQND7XMCI35V4LJ/bundle.json","state_url":"https://pith.science/pith/YNNCXTBJ76FYQND7XMCI35V4LJ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/YNNCXTBJ76FYQND7XMCI35V4LJ/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":"2026-06-11T11:13:44Z","links":{"resolver":"https://pith.science/pith/YNNCXTBJ76FYQND7XMCI35V4LJ","bundle":"https://pith.science/pith/YNNCXTBJ76FYQND7XMCI35V4LJ/bundle.json","state":"https://pith.science/pith/YNNCXTBJ76FYQND7XMCI35V4LJ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/YNNCXTBJ76FYQND7XMCI35V4LJ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:YNNCXTBJ76FYQND7XMCI35V4LJ","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":"06759393cf8c969ac1725427504173ab94135519f94cd904e219e781ddb7adc9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-07T10:29:59Z","title_canon_sha256":"4a586b146ebee6c7e03a28d11bec4687e85c001d4fce87ba9bfd67778c83fa1c"},"schema_version":"1.0","source":{"id":"1301.1147","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1301.1147","created_at":"2026-05-18T01:52:21Z"},{"alias_kind":"arxiv_version","alias_value":"1301.1147v2","created_at":"2026-05-18T01:52:21Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1301.1147","created_at":"2026-05-18T01:52:21Z"},{"alias_kind":"pith_short_12","alias_value":"YNNCXTBJ76FY","created_at":"2026-05-18T12:28:06Z"},{"alias_kind":"pith_short_16","alias_value":"YNNCXTBJ76FYQND7","created_at":"2026-05-18T12:28:06Z"},{"alias_kind":"pith_short_8","alias_value":"YNNCXTBJ","created_at":"2026-05-18T12:28:06Z"}],"graph_snapshots":[{"event_id":"sha256:4c7078317c7d05eccf85aa6f9355bee5fd896fc20866f24bfa25e5864385ef1a","target":"graph","created_at":"2026-05-18T01:52:21Z","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":"Context. There have been a long string of efforts to understand the source of the variability observed in microquasars, especially concerning the elusive High-Frequency Quasi-Periodic Oscillation. These oscillations are among the fastest phenomena that affect matter in the vicinity of stellar black holes and therefore could be used as probes of strong-field general relativity. Nevertheless, no model has yet gained wide acceptance. Aims. The aim of this article is to investigate the model derived from the occurrence of the Rossby wave instability at the inner edge of the accretion disk. In part","authors_text":"F. H. Vincent, H. Meheut, P. Varniere, T. Paumard","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-07T10:29:59Z","title":"Flux Modulation from the Rossby Wave Instability in microquasars accretion disks: toward a HFQPO model"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1301.1147","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:d2698307e8d45d39df20146bbe5090f9340e0f8c03278136f41e7c41e7c83564","target":"record","created_at":"2026-05-18T01:52:21Z","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":"06759393cf8c969ac1725427504173ab94135519f94cd904e219e781ddb7adc9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-01-07T10:29:59Z","title_canon_sha256":"4a586b146ebee6c7e03a28d11bec4687e85c001d4fce87ba9bfd67778c83fa1c"},"schema_version":"1.0","source":{"id":"1301.1147","kind":"arxiv","version":2}},"canonical_sha256":"c35a2bcc29ff8b88347fbb048df6bc5a7d0f0c4311ee24d10a3c0a499d5c1e4c","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"c35a2bcc29ff8b88347fbb048df6bc5a7d0f0c4311ee24d10a3c0a499d5c1e4c","first_computed_at":"2026-05-18T01:52:21.142505Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:52:21.142505Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"KgQIHXWFYiVcPGwKQFreZAxOh2valtiEVVrWhJDQZG5MpniwWvwKbXGueuSIKOO/oNiNz28F8lK5bMrQ4l/JAg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:52:21.142912Z","signed_message":"canonical_sha256_bytes"},"source_id":"1301.1147","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:d2698307e8d45d39df20146bbe5090f9340e0f8c03278136f41e7c41e7c83564","sha256:4c7078317c7d05eccf85aa6f9355bee5fd896fc20866f24bfa25e5864385ef1a"],"state_sha256":"46519ebd4f5b6e11da79c79e8c04e8a26141df4c9e20c7a868677fc4635100ba"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"iyEGvgf48QvyvoAtUty7iznkvmJbP7/FZ2gVDwJ5TiCSAhlewslxINn03rWixJzqrmnLGUa3BBGiTs6h3S/+Aw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-11T11:13:44.160926Z","bundle_sha256":"2174f6e7d8d7de87156ef0102f4f6b6a15bc4c4c6e9583a8bad586ceed81f9d3"}}