{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:VFU6PZDTV5DWZCWYWPGFDWNNQ4","short_pith_number":"pith:VFU6PZDT","canonical_record":{"source":{"id":"1710.01590","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-04T13:14:26Z","cross_cats_sorted":[],"title_canon_sha256":"aef9f8731a36e8fafe6cd9c7c0ad33da1cdd8db559e260de256802f63558aa67","abstract_canon_sha256":"ac881af82b819279bc744a5a1fe0c0e3c04a6539e9f5f99fadd266be2caf8705"},"schema_version":"1.0"},"canonical_sha256":"a969e7e473af476c8ad8b3cc51d9ad87248a41040f136872ef8af218764386f7","source":{"kind":"arxiv","id":"1710.01590","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1710.01590","created_at":"2026-05-18T00:30:40Z"},{"alias_kind":"arxiv_version","alias_value":"1710.01590v1","created_at":"2026-05-18T00:30:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.01590","created_at":"2026-05-18T00:30:40Z"},{"alias_kind":"pith_short_12","alias_value":"VFU6PZDTV5DW","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_16","alias_value":"VFU6PZDTV5DWZCWY","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_8","alias_value":"VFU6PZDT","created_at":"2026-05-18T12:31:49Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:VFU6PZDTV5DWZCWYWPGFDWNNQ4","target":"record","payload":{"canonical_record":{"source":{"id":"1710.01590","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-04T13:14:26Z","cross_cats_sorted":[],"title_canon_sha256":"aef9f8731a36e8fafe6cd9c7c0ad33da1cdd8db559e260de256802f63558aa67","abstract_canon_sha256":"ac881af82b819279bc744a5a1fe0c0e3c04a6539e9f5f99fadd266be2caf8705"},"schema_version":"1.0"},"canonical_sha256":"a969e7e473af476c8ad8b3cc51d9ad87248a41040f136872ef8af218764386f7","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:30:40.814887Z","signature_b64":"RWYSXX8FHgLpDkIj0V/Jz0oVMkWOKsE1TgtmBKvTRRLu9Va6f9bh+dTnYkdDEy1LFW9A+6Ssct4ywULOhFNKBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a969e7e473af476c8ad8b3cc51d9ad87248a41040f136872ef8af218764386f7","last_reissued_at":"2026-05-18T00:30:40.814366Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:30:40.814366Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1710.01590","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":"2026-05-18T00:30:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2v1tEgzXJ8kY2A9HcV2tKethb+jH+2eoT9TH3J9Y86CP5aGe5Ijb3oVCVT58Fw3sAZgNiXMtYrj+0fEA0ByZAg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-30T08:17:14.521598Z"},"content_sha256":"570889ab3817b22e418dd81fb6514b1798e5e01363e1268b0a51f23750b1d537","schema_version":"1.0","event_id":"sha256:570889ab3817b22e418dd81fb6514b1798e5e01363e1268b0a51f23750b1d537"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:VFU6PZDTV5DWZCWYWPGFDWNNQ4","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Parallel tracks as quasi-steady states for the magnetic boundary layers in neutron-star low-mass X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"M. Hakan Erkut, Onur \\c{C}atmabacak","submitted_at":"2017-10-04T13:14:26Z","abstract_excerpt":"The neutron stars in low-mass X-ray binaries (LMXBs) are usually thought to be weakly magnetized objects accreting matter from their low-mass companions in the form of a disk. Albeit weak as compared to those in young neutron-star systems, the neutron-star magnetospheres in LMXBs can play an important role in determining the correlations between spectral and temporal properties. Parallel tracks appearing in the plane of kilohertz (kHz) quasi-periodic oscillation (QPO) frequency versus X-ray flux can be used as a tool to study the magnetosphere-disk interaction in neutron-star LMXBs. For dynami"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.01590","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":"2026-05-18T00:30:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"YZwP8H4CzmihlQevwYIueFX96uGeGAvSlSazwDRCA0KVeiQvQxJtF6GOeLCM8wK6ov70hZvZqg6BArREFuyDCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-30T08:17:14.521935Z"},"content_sha256":"f048dcd37207b324694e20e1d7cde9a64e76c661dc1bef3970d10f3272211242","schema_version":"1.0","event_id":"sha256:f048dcd37207b324694e20e1d7cde9a64e76c661dc1bef3970d10f3272211242"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VFU6PZDTV5DWZCWYWPGFDWNNQ4/bundle.json","state_url":"https://pith.science/pith/VFU6PZDTV5DWZCWYWPGFDWNNQ4/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VFU6PZDTV5DWZCWYWPGFDWNNQ4/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":"2026-06-30T08:17:14Z","links":{"resolver":"https://pith.science/pith/VFU6PZDTV5DWZCWYWPGFDWNNQ4","bundle":"https://pith.science/pith/VFU6PZDTV5DWZCWYWPGFDWNNQ4/bundle.json","state":"https://pith.science/pith/VFU6PZDTV5DWZCWYWPGFDWNNQ4/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VFU6PZDTV5DWZCWYWPGFDWNNQ4/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:VFU6PZDTV5DWZCWYWPGFDWNNQ4","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":"ac881af82b819279bc744a5a1fe0c0e3c04a6539e9f5f99fadd266be2caf8705","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-04T13:14:26Z","title_canon_sha256":"aef9f8731a36e8fafe6cd9c7c0ad33da1cdd8db559e260de256802f63558aa67"},"schema_version":"1.0","source":{"id":"1710.01590","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1710.01590","created_at":"2026-05-18T00:30:40Z"},{"alias_kind":"arxiv_version","alias_value":"1710.01590v1","created_at":"2026-05-18T00:30:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.01590","created_at":"2026-05-18T00:30:40Z"},{"alias_kind":"pith_short_12","alias_value":"VFU6PZDTV5DW","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_16","alias_value":"VFU6PZDTV5DWZCWY","created_at":"2026-05-18T12:31:49Z"},{"alias_kind":"pith_short_8","alias_value":"VFU6PZDT","created_at":"2026-05-18T12:31:49Z"}],"graph_snapshots":[{"event_id":"sha256:f048dcd37207b324694e20e1d7cde9a64e76c661dc1bef3970d10f3272211242","target":"graph","created_at":"2026-05-18T00:30:40Z","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 neutron stars in low-mass X-ray binaries (LMXBs) are usually thought to be weakly magnetized objects accreting matter from their low-mass companions in the form of a disk. Albeit weak as compared to those in young neutron-star systems, the neutron-star magnetospheres in LMXBs can play an important role in determining the correlations between spectral and temporal properties. Parallel tracks appearing in the plane of kilohertz (kHz) quasi-periodic oscillation (QPO) frequency versus X-ray flux can be used as a tool to study the magnetosphere-disk interaction in neutron-star LMXBs. For dynami","authors_text":"M. Hakan Erkut, Onur \\c{C}atmabacak","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-04T13:14:26Z","title":"Parallel tracks as quasi-steady states for the magnetic boundary layers in neutron-star low-mass X-ray binaries"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.01590","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":"sha256:570889ab3817b22e418dd81fb6514b1798e5e01363e1268b0a51f23750b1d537","target":"record","created_at":"2026-05-18T00:30:40Z","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":"ac881af82b819279bc744a5a1fe0c0e3c04a6539e9f5f99fadd266be2caf8705","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-04T13:14:26Z","title_canon_sha256":"aef9f8731a36e8fafe6cd9c7c0ad33da1cdd8db559e260de256802f63558aa67"},"schema_version":"1.0","source":{"id":"1710.01590","kind":"arxiv","version":1}},"canonical_sha256":"a969e7e473af476c8ad8b3cc51d9ad87248a41040f136872ef8af218764386f7","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"a969e7e473af476c8ad8b3cc51d9ad87248a41040f136872ef8af218764386f7","first_computed_at":"2026-05-18T00:30:40.814366Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:30:40.814366Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"RWYSXX8FHgLpDkIj0V/Jz0oVMkWOKsE1TgtmBKvTRRLu9Va6f9bh+dTnYkdDEy1LFW9A+6Ssct4ywULOhFNKBQ==","signature_status":"signed_v1","signed_at":"2026-05-18T00:30:40.814887Z","signed_message":"canonical_sha256_bytes"},"source_id":"1710.01590","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:570889ab3817b22e418dd81fb6514b1798e5e01363e1268b0a51f23750b1d537","sha256:f048dcd37207b324694e20e1d7cde9a64e76c661dc1bef3970d10f3272211242"],"state_sha256":"655af751102e08d5be980573493484e32990fcbeaaa96d1a492f40423866f31d"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Ww8j2mq2rwTnpBhKY2hqhhGw5w6g0fLf0gzCtWu4wvbzgl+ylntlGts6ZpDZaYQIKb1kGGtK1n2UpGKda+/uBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-30T08:17:14.523956Z","bundle_sha256":"0e22d8bc9dec2000c8b0a13a66b7ae62958fe35c5aaacbdc71d0038c483ee2e4"}}