{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:LF5VW3MAO4DX2XH5OHYQJFM5T7","short_pith_number":"pith:LF5VW3MA","canonical_record":{"source":{"id":"1212.0866","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-12-04T21:02:29Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"6391b86f624f389fbd70ce4ebd23acfa90f373cde0f67064dc16620803d092cf","abstract_canon_sha256":"d41390c8078be1ca9c5722faa456f14ac067846ed8ad1c6193a0404b5b3927a7"},"schema_version":"1.0"},"canonical_sha256":"597b5b6d8077077d5cfd71f104959d9ff4e40aa80675402f83f06dc24ac55400","source":{"kind":"arxiv","id":"1212.0866","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1212.0866","created_at":"2026-05-18T01:52:47Z"},{"alias_kind":"arxiv_version","alias_value":"1212.0866v1","created_at":"2026-05-18T01:52:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1212.0866","created_at":"2026-05-18T01:52:47Z"},{"alias_kind":"pith_short_12","alias_value":"LF5VW3MAO4DX","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_16","alias_value":"LF5VW3MAO4DX2XH5","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_8","alias_value":"LF5VW3MA","created_at":"2026-05-18T12:27:14Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:LF5VW3MAO4DX2XH5OHYQJFM5T7","target":"record","payload":{"canonical_record":{"source":{"id":"1212.0866","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-12-04T21:02:29Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"6391b86f624f389fbd70ce4ebd23acfa90f373cde0f67064dc16620803d092cf","abstract_canon_sha256":"d41390c8078be1ca9c5722faa456f14ac067846ed8ad1c6193a0404b5b3927a7"},"schema_version":"1.0"},"canonical_sha256":"597b5b6d8077077d5cfd71f104959d9ff4e40aa80675402f83f06dc24ac55400","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:52:47.680469Z","signature_b64":"Z/pzxvE39Dn7O+pZJOmwTXhM4+SGpY6QKAV/Ld37UwhvHKN+5DsJ3K0RDaduobBtN3eM9/hBio+R+Y/eRQiHBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"597b5b6d8077077d5cfd71f104959d9ff4e40aa80675402f83f06dc24ac55400","last_reissued_at":"2026-05-18T01:52:47.679951Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:52:47.679951Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1212.0866","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":"2026-05-18T01:52:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"NQH8cokGoizcK3W9Ce1/5x+XiAr9ukmb6E1Pnm2cpPyAneNfHwkHQXJ0hUhs81AkN3FTN31CMYnwliOLwt4qAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T08:55:00.111264Z"},"content_sha256":"2bc1cfc250cc400154923dd944138911d108c3158b2a046c342fc4d2aa934d06","schema_version":"1.0","event_id":"sha256:2bc1cfc250cc400154923dd944138911d108c3158b2a046c342fc4d2aa934d06"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:LF5VW3MAO4DX2XH5OHYQJFM5T7","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Relations between X-ray timing features and spectral parameters of Galactic black hole X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"(2) Sabanc{\\i} \\\"Universitesi, (3) ESAC/ESA), E. Kalemci (2), H. Stiele (1), S. Motta (3) ((1) INAF-OAB, T. M. Belloni (1)","submitted_at":"2012-12-04T21:02:29Z","abstract_excerpt":"We present a study of correlations between spectral and timing parameters for a sample of black hole X-ray binary candidates. Data are taken from GX 339-4, H 1743-322, and XTE J1650-500, as the Rossi X-ray Timing Explorer (RXTE) observed complete outbursts of these sources. In our study we investigate outbursts that happened before the end of 2009 to make use of the high-energy coverage of the HEXTE detector and select observations that show a certain type of quasi-periodic oscillations (type-C QPOs). The spectral parameters are derived using the empirical convolution model simpl to model the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1212.0866","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":"2026-05-18T01:52:47Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"UbN/JEXew4PJYOjI5eo5UHreQBxozh34kYqKiaqx3pkMRG+5ugK8p/AklFEpy4AhT7EdNr+r0GK0o6YNh+6NCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T08:55:00.112116Z"},"content_sha256":"cc53d84fbbd03811bc5815b153e3c87d952be9fc1c48257f49b668e6b630ec1c","schema_version":"1.0","event_id":"sha256:cc53d84fbbd03811bc5815b153e3c87d952be9fc1c48257f49b668e6b630ec1c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/LF5VW3MAO4DX2XH5OHYQJFM5T7/bundle.json","state_url":"https://pith.science/pith/LF5VW3MAO4DX2XH5OHYQJFM5T7/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/LF5VW3MAO4DX2XH5OHYQJFM5T7/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":"2026-05-27T08:55:00Z","links":{"resolver":"https://pith.science/pith/LF5VW3MAO4DX2XH5OHYQJFM5T7","bundle":"https://pith.science/pith/LF5VW3MAO4DX2XH5OHYQJFM5T7/bundle.json","state":"https://pith.science/pith/LF5VW3MAO4DX2XH5OHYQJFM5T7/state.json","well_known_bundle":"https://pith.science/.well-known/pith/LF5VW3MAO4DX2XH5OHYQJFM5T7/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:LF5VW3MAO4DX2XH5OHYQJFM5T7","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":"d41390c8078be1ca9c5722faa456f14ac067846ed8ad1c6193a0404b5b3927a7","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-12-04T21:02:29Z","title_canon_sha256":"6391b86f624f389fbd70ce4ebd23acfa90f373cde0f67064dc16620803d092cf"},"schema_version":"1.0","source":{"id":"1212.0866","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1212.0866","created_at":"2026-05-18T01:52:47Z"},{"alias_kind":"arxiv_version","alias_value":"1212.0866v1","created_at":"2026-05-18T01:52:47Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1212.0866","created_at":"2026-05-18T01:52:47Z"},{"alias_kind":"pith_short_12","alias_value":"LF5VW3MAO4DX","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_16","alias_value":"LF5VW3MAO4DX2XH5","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_8","alias_value":"LF5VW3MA","created_at":"2026-05-18T12:27:14Z"}],"graph_snapshots":[{"event_id":"sha256:cc53d84fbbd03811bc5815b153e3c87d952be9fc1c48257f49b668e6b630ec1c","target":"graph","created_at":"2026-05-18T01:52:47Z","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":"We present a study of correlations between spectral and timing parameters for a sample of black hole X-ray binary candidates. Data are taken from GX 339-4, H 1743-322, and XTE J1650-500, as the Rossi X-ray Timing Explorer (RXTE) observed complete outbursts of these sources. In our study we investigate outbursts that happened before the end of 2009 to make use of the high-energy coverage of the HEXTE detector and select observations that show a certain type of quasi-periodic oscillations (type-C QPOs). The spectral parameters are derived using the empirical convolution model simpl to model the ","authors_text":"(2) Sabanc{\\i} \\\"Universitesi, (3) ESAC/ESA), E. Kalemci (2), H. Stiele (1), S. Motta (3) ((1) INAF-OAB, T. M. Belloni (1)","cross_cats":["astro-ph.GA"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-12-04T21:02:29Z","title":"Relations between X-ray timing features and spectral parameters of Galactic black hole X-ray binaries"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1212.0866","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":"sha256:2bc1cfc250cc400154923dd944138911d108c3158b2a046c342fc4d2aa934d06","target":"record","created_at":"2026-05-18T01:52:47Z","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":"d41390c8078be1ca9c5722faa456f14ac067846ed8ad1c6193a0404b5b3927a7","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-12-04T21:02:29Z","title_canon_sha256":"6391b86f624f389fbd70ce4ebd23acfa90f373cde0f67064dc16620803d092cf"},"schema_version":"1.0","source":{"id":"1212.0866","kind":"arxiv","version":1}},"canonical_sha256":"597b5b6d8077077d5cfd71f104959d9ff4e40aa80675402f83f06dc24ac55400","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"597b5b6d8077077d5cfd71f104959d9ff4e40aa80675402f83f06dc24ac55400","first_computed_at":"2026-05-18T01:52:47.679951Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:52:47.679951Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Z/pzxvE39Dn7O+pZJOmwTXhM4+SGpY6QKAV/Ld37UwhvHKN+5DsJ3K0RDaduobBtN3eM9/hBio+R+Y/eRQiHBg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:52:47.680469Z","signed_message":"canonical_sha256_bytes"},"source_id":"1212.0866","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:2bc1cfc250cc400154923dd944138911d108c3158b2a046c342fc4d2aa934d06","sha256:cc53d84fbbd03811bc5815b153e3c87d952be9fc1c48257f49b668e6b630ec1c"],"state_sha256":"8c29feecbb6d0f3942e8d495a2fffa795469fecf4301ac59a7a9cff3add3901d"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AF1fP4aa+FN2s/87epobxYhp3r7/F6lQ4xJaIckwCKr6kMHlEzD2vKJ/U7WGYwxo+s6qIT5CevSqmsH8uoXbBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T08:55:00.115286Z","bundle_sha256":"9c90c8f26fdc1e44b28e55b7829874aa2b14c2efba5c255bb556a1fc533538b6"}}