{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:NYJFEJOUM3SDSI6AME23F2IEC7","short_pith_number":"pith:NYJFEJOU","schema_version":"1.0","canonical_sha256":"6e125225d466e43923c06135b2e90417db855ec68083442a135f579af41a7c43","source":{"kind":"arxiv","id":"1308.0919","version":1},"attestation_state":"computed","paper":{"title":"Detection of a variable QPO at ~41 mHz in the Be/X-ray transient pulsar 4U 0115+634","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Ahmedabad), Astrophysics Division, Astrophysics Laboratory, Department of Physics, Gaurava K. Jaisawal (2), Mohanlal Sukhadia University, Moti R. Dugair (1), Navrangapura, Physical Research Laboratory, Sachindra Naik (2), S. N. A. Jaaffrey (1) ((1) Astronomy, Udaipur (2) Astronomy","submitted_at":"2013-08-05T09:40:23Z","abstract_excerpt":"We report the detection of quasi-periodic oscillation (QPO) at ~41 mHz in the transient high-mass Be/X-ray binary pulsar 4U~0115+634 using data from the Rossi X-Ray Timing Explorer (RXTE) observatory. The observations used in the present work were carried out during X-ray outbursts in 1999 March-April, 2004 September-October and 2008 March-April. This frequency of the newly detected QPO was found to vary in 27-46 mHz range. This ~41 mHz QPO was detected in four of the 36 pointed RXTE Proportional Counter Array (PCA) observations during 1999 outburst where as during 2004 and 2008 outbursts, it "},"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":"1308.0919","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-08-05T09:40:23Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"40f373fe1a786583e352d9415af6daa9eaa714b829ec18140a04df8fac36e930","abstract_canon_sha256":"012962c80cb6aaa0095dbf01bc03e0af5e4a7168fbb7115869ea50f6ea78df46"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:20:50.816566Z","signature_b64":"NKX0dzR337hQ0YKSqS8g1DmjrhKPFzFR5lC5El9WB3UOyO4YsSABH0fY5TRrXOlgb+ccRP1gvVzAmHaD0uoXAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6e125225d466e43923c06135b2e90417db855ec68083442a135f579af41a7c43","last_reissued_at":"2026-05-18T01:20:50.816004Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:20:50.816004Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection of a variable QPO at ~41 mHz in the Be/X-ray transient pulsar 4U 0115+634","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Ahmedabad), Astrophysics Division, Astrophysics Laboratory, Department of Physics, Gaurava K. Jaisawal (2), Mohanlal Sukhadia University, Moti R. Dugair (1), Navrangapura, Physical Research Laboratory, Sachindra Naik (2), S. N. A. Jaaffrey (1) ((1) Astronomy, Udaipur (2) Astronomy","submitted_at":"2013-08-05T09:40:23Z","abstract_excerpt":"We report the detection of quasi-periodic oscillation (QPO) at ~41 mHz in the transient high-mass Be/X-ray binary pulsar 4U~0115+634 using data from the Rossi X-Ray Timing Explorer (RXTE) observatory. The observations used in the present work were carried out during X-ray outbursts in 1999 March-April, 2004 September-October and 2008 March-April. This frequency of the newly detected QPO was found to vary in 27-46 mHz range. This ~41 mHz QPO was detected in four of the 36 pointed RXTE Proportional Counter Array (PCA) observations during 1999 outburst where as during 2004 and 2008 outbursts, it "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.0919","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1308.0919","created_at":"2026-05-18T01:20:50.816081+00:00"},{"alias_kind":"arxiv_version","alias_value":"1308.0919v1","created_at":"2026-05-18T01:20:50.816081+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.0919","created_at":"2026-05-18T01:20:50.816081+00:00"},{"alias_kind":"pith_short_12","alias_value":"NYJFEJOUM3SD","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_16","alias_value":"NYJFEJOUM3SDSI6A","created_at":"2026-05-18T12:27:52.871228+00:00"},{"alias_kind":"pith_short_8","alias_value":"NYJFEJOU","created_at":"2026-05-18T12:27:52.871228+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7","json":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7.json","graph_json":"https://pith.science/api/pith-number/NYJFEJOUM3SDSI6AME23F2IEC7/graph.json","events_json":"https://pith.science/api/pith-number/NYJFEJOUM3SDSI6AME23F2IEC7/events.json","paper":"https://pith.science/paper/NYJFEJOU"},"agent_actions":{"view_html":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7","download_json":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7.json","view_paper":"https://pith.science/paper/NYJFEJOU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1308.0919&json=true","fetch_graph":"https://pith.science/api/pith-number/NYJFEJOUM3SDSI6AME23F2IEC7/graph.json","fetch_events":"https://pith.science/api/pith-number/NYJFEJOUM3SDSI6AME23F2IEC7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7/action/storage_attestation","attest_author":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7/action/author_attestation","sign_citation":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7/action/citation_signature","submit_replication":"https://pith.science/pith/NYJFEJOUM3SDSI6AME23F2IEC7/action/replication_record"}},"created_at":"2026-05-18T01:20:50.816081+00:00","updated_at":"2026-05-18T01:20:50.816081+00:00"}