{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:E4JDS7P3EUDQ2DYFIXZRP2G5YQ","short_pith_number":"pith:E4JDS7P3","schema_version":"1.0","canonical_sha256":"2712397dfb25070d0f0545f317e8ddc41dbb9d7293b2bca6f5ccbd12cb4ee220","source":{"kind":"arxiv","id":"astro-ph/0611716","version":2},"attestation_state":"computed","paper":{"title":"Evidence for 1122 Hz X-Ray Burst Oscillations from the Neutron-Star X-Ray Transient XTE J1739-285","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Gotz, E. Kuulkers, J.A. Tomsick, J.J.M. in 't Zand, N. Lund, P. Kaaret, S. Brandt, S. Mereghetti, Z. Prieskorn","submitted_at":"2006-11-22T16:16:01Z","abstract_excerpt":"We report on millisecond variability from the X-ray transient XTE J1739-285. We detected six X-ray type I bursts and found evidence for oscillations at 1122 +/- 0.3 Hz in the brightest X-ray burst. Taking into consideration the power in the oscillations and the number of trials in the search, the detection is significant at the 99.96% confidence level. If the oscillations are confirmed, the oscillation frequency would suggest that XTE J1739-285 contains the fastest rotating neutron star yet found. We also found millisecond quasiperiodic oscillations in the persistent emission with frequencies "},"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":"astro-ph/0611716","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-11-22T16:16:01Z","cross_cats_sorted":[],"title_canon_sha256":"7f924229203a7a1acb6b904c42ac6f9efce8da5a543933590dc738c52b719d1c","abstract_canon_sha256":"7f798d870e36d2f8b16387d3547e3b656f1c1d95212f456a6faf8094fd3a48eb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:59:40.717358Z","signature_b64":"xe+zZYpARJCNAaHVEgyXHK+QK3KbZdmk6WxFBHu+nwpUvgLp7a9JNusbudxF+Gt6P4ZqtajMhsQvkeohyOTXDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2712397dfb25070d0f0545f317e8ddc41dbb9d7293b2bca6f5ccbd12cb4ee220","last_reissued_at":"2026-07-04T16:59:40.716843Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:59:40.716843Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Evidence for 1122 Hz X-Ray Burst Oscillations from the Neutron-Star X-Ray Transient XTE J1739-285","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Gotz, E. Kuulkers, J.A. Tomsick, J.J.M. in 't Zand, N. Lund, P. Kaaret, S. Brandt, S. Mereghetti, Z. Prieskorn","submitted_at":"2006-11-22T16:16:01Z","abstract_excerpt":"We report on millisecond variability from the X-ray transient XTE J1739-285. We detected six X-ray type I bursts and found evidence for oscillations at 1122 +/- 0.3 Hz in the brightest X-ray burst. Taking into consideration the power in the oscillations and the number of trials in the search, the detection is significant at the 99.96% confidence level. If the oscillations are confirmed, the oscillation frequency would suggest that XTE J1739-285 contains the fastest rotating neutron star yet found. We also found millisecond quasiperiodic oscillations in the persistent emission with frequencies "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0611716","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0611716/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"astro-ph/0611716","created_at":"2026-07-04T16:59:40.716900+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0611716v2","created_at":"2026-07-04T16:59:40.716900+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0611716","created_at":"2026-07-04T16:59:40.716900+00:00"},{"alias_kind":"pith_short_12","alias_value":"E4JDS7P3EUDQ","created_at":"2026-07-04T16:59:40.716900+00:00"},{"alias_kind":"pith_short_16","alias_value":"E4JDS7P3EUDQ2DYF","created_at":"2026-07-04T16:59:40.716900+00:00"},{"alias_kind":"pith_short_8","alias_value":"E4JDS7P3","created_at":"2026-07-04T16:59:40.716900+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.06578","citing_title":"A Disappearing Act: Constraints From \"Missing\" Flares of Repeating Partial TDE Candidates","ref_index":142,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ","json":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ.json","graph_json":"https://pith.science/api/pith-number/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/graph.json","events_json":"https://pith.science/api/pith-number/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/events.json","paper":"https://pith.science/paper/E4JDS7P3"},"agent_actions":{"view_html":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ","download_json":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ.json","view_paper":"https://pith.science/paper/E4JDS7P3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0611716&json=true","fetch_graph":"https://pith.science/api/pith-number/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/graph.json","fetch_events":"https://pith.science/api/pith-number/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/action/storage_attestation","attest_author":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/action/author_attestation","sign_citation":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/action/citation_signature","submit_replication":"https://pith.science/pith/E4JDS7P3EUDQ2DYFIXZRP2G5YQ/action/replication_record"}},"created_at":"2026-07-04T16:59:40.716900+00:00","updated_at":"2026-07-04T16:59:40.716900+00:00"}