{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:NLKVY3GMC7XD65X3WNFTTGAOGC","short_pith_number":"pith:NLKVY3GM","schema_version":"1.0","canonical_sha256":"6ad55c6ccc17ee3f76fbb34b39980e30927c0c9ca2e05341609bf7d7e598f0df","source":{"kind":"arxiv","id":"1408.5146","version":2},"attestation_state":"computed","paper":{"title":"X-ray outbursts of low-mass X-ray binary transients observed in the RXTE era","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Wenfei Yu, Zhen Yan","submitted_at":"2014-08-21T20:02:08Z","abstract_excerpt":"We have performed a statistical study of the properties of 110 bright X-ray outbursts in 36 low-mass X-ray binary transients (LMXBTs) seen with the All-Sky Monitor (2--12 keV) on board the {\\it Rossi X-ray Timing Explorer} ({\\it RXTE}) in 1996--2011. We have measured a number of outburst properties, including peak X-ray luminosity, rate of change of luminosity on a daily timescale, $e$-folding rise and decay timescales, outburst duration, and total radiated energy. We found that the average properties such as peak X-ray luminosity, rise and decay timescales, outburst duration, and total radiat"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1408.5146","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-08-21T20:02:08Z","cross_cats_sorted":[],"title_canon_sha256":"de0438f64b8ca2e6ea4618bb29d44827054d979e343252c1dd910f38c894a68a","abstract_canon_sha256":"c93bcfcbbdd996567654f4819fc1968004c0d8dfa515bf6418a1e4540da11077"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:37.416100Z","signature_b64":"sVFdg20JHAj4jhaoYxP7fqMO7tOo+AbSONztb2sll6xSTC9XQB0crTfNNd2bFdZ87QFcEP/3Or4I9mrdb69rBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6ad55c6ccc17ee3f76fbb34b39980e30927c0c9ca2e05341609bf7d7e598f0df","last_reissued_at":"2026-05-18T02:03:37.415533Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:37.415533Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"X-ray outbursts of low-mass X-ray binary transients observed in the RXTE era","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Wenfei Yu, Zhen Yan","submitted_at":"2014-08-21T20:02:08Z","abstract_excerpt":"We have performed a statistical study of the properties of 110 bright X-ray outbursts in 36 low-mass X-ray binary transients (LMXBTs) seen with the All-Sky Monitor (2--12 keV) on board the {\\it Rossi X-ray Timing Explorer} ({\\it RXTE}) in 1996--2011. We have measured a number of outburst properties, including peak X-ray luminosity, rate of change of luminosity on a daily timescale, $e$-folding rise and decay timescales, outburst duration, and total radiated energy. We found that the average properties such as peak X-ray luminosity, rise and decay timescales, outburst duration, and total radiat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.5146","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1408.5146","created_at":"2026-05-18T02:03:37.415634+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.5146v2","created_at":"2026-05-18T02:03:37.415634+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.5146","created_at":"2026-05-18T02:03:37.415634+00:00"},{"alias_kind":"pith_short_12","alias_value":"NLKVY3GMC7XD","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_16","alias_value":"NLKVY3GMC7XD65X3","created_at":"2026-05-18T12:28:41.024544+00:00"},{"alias_kind":"pith_short_8","alias_value":"NLKVY3GM","created_at":"2026-05-18T12:28:41.024544+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.19473","citing_title":"Radio-X-ray Time Lags in GX 339-4: Probing Magnetic Field Transport in Black Hole Accretion","ref_index":18,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC","json":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC.json","graph_json":"https://pith.science/api/pith-number/NLKVY3GMC7XD65X3WNFTTGAOGC/graph.json","events_json":"https://pith.science/api/pith-number/NLKVY3GMC7XD65X3WNFTTGAOGC/events.json","paper":"https://pith.science/paper/NLKVY3GM"},"agent_actions":{"view_html":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC","download_json":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC.json","view_paper":"https://pith.science/paper/NLKVY3GM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.5146&json=true","fetch_graph":"https://pith.science/api/pith-number/NLKVY3GMC7XD65X3WNFTTGAOGC/graph.json","fetch_events":"https://pith.science/api/pith-number/NLKVY3GMC7XD65X3WNFTTGAOGC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC/action/storage_attestation","attest_author":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC/action/author_attestation","sign_citation":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC/action/citation_signature","submit_replication":"https://pith.science/pith/NLKVY3GMC7XD65X3WNFTTGAOGC/action/replication_record"}},"created_at":"2026-05-18T02:03:37.415634+00:00","updated_at":"2026-05-18T02:03:37.415634+00:00"}