{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:6GQ7DDUBEQIA7ZQ6RRBXFIO6WX","short_pith_number":"pith:6GQ7DDUB","schema_version":"1.0","canonical_sha256":"f1a1f18e8124100fe61e8c4372a1deb5e1a87cc27892f778115890dd6e2fd3e6","source":{"kind":"arxiv","id":"2401.11134","version":1},"attestation_state":"computed","paper":{"title":"Detection of Solar-like Oscillations in Sub-giant and Red Giant Stars Using 2-minute Cadence TESS Data","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Jianzhao Zhou, Jie Yu, Lifei Ye, Liu Long, Mengjie Li, Shaolan Bi, Tanda Li, Tiancheng Sun, Xianfei Zhang, Yaguang Li","submitted_at":"2024-01-20T06:13:11Z","abstract_excerpt":"Based on all 2-minute cadence $TESS$ light curves from Sector 1 to 60, we provide a catalog of 8,651 solar-like oscillators, including frequency at maximum power ($\\nu_{\\rm max}$, with its median precision, $\\sigma$=5.39\\%), large frequency separation ($\\Delta\\nu$, $\\sigma$=6.22\\%), seismically derived masses, radii, and surface gravity. In this sample, we have detected 2,173 new oscillators and added 4,373 new $\\Delta\\nu$ measurements. Our seismic parameters are consistent with those from $Kepler$, $K2$, and previous $TESS$ data. The median fractional residual in $\\nu_{\\rm max}$ is $1.63\\%$ w"},"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":"2401.11134","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-01-20T06:13:11Z","cross_cats_sorted":["astro-ph.EP"],"title_canon_sha256":"83e33412b48b54e43c7bd76dcbf779c624e50672c972ecf879abe16971e2f487","abstract_canon_sha256":"14e5b4a8c5c00b619fe9a29bba91001647378c9baac29bee47f03f75b035d150"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:35:46.383233Z","signature_b64":"SGegfEY/APGqo58Dn1DhlpESuVTNvLcwcPDY/JWlclWFpnKT+VUAdZu5H/Qg+k8lnUT9qZ4dnRPlH88/h32XAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1a1f18e8124100fe61e8c4372a1deb5e1a87cc27892f778115890dd6e2fd3e6","last_reissued_at":"2026-07-05T07:35:46.382729Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:35:46.382729Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detection of Solar-like Oscillations in Sub-giant and Red Giant Stars Using 2-minute Cadence TESS Data","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.EP"],"primary_cat":"astro-ph.SR","authors_text":"Jianzhao Zhou, Jie Yu, Lifei Ye, Liu Long, Mengjie Li, Shaolan Bi, Tanda Li, Tiancheng Sun, Xianfei Zhang, Yaguang Li","submitted_at":"2024-01-20T06:13:11Z","abstract_excerpt":"Based on all 2-minute cadence $TESS$ light curves from Sector 1 to 60, we provide a catalog of 8,651 solar-like oscillators, including frequency at maximum power ($\\nu_{\\rm max}$, with its median precision, $\\sigma$=5.39\\%), large frequency separation ($\\Delta\\nu$, $\\sigma$=6.22\\%), seismically derived masses, radii, and surface gravity. In this sample, we have detected 2,173 new oscillators and added 4,373 new $\\Delta\\nu$ measurements. Our seismic parameters are consistent with those from $Kepler$, $K2$, and previous $TESS$ data. The median fractional residual in $\\nu_{\\rm max}$ is $1.63\\%$ w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2401.11134","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2401.11134/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":"2401.11134","created_at":"2026-07-05T07:35:46.382784+00:00"},{"alias_kind":"arxiv_version","alias_value":"2401.11134v1","created_at":"2026-07-05T07:35:46.382784+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2401.11134","created_at":"2026-07-05T07:35:46.382784+00:00"},{"alias_kind":"pith_short_12","alias_value":"6GQ7DDUBEQIA","created_at":"2026-07-05T07:35:46.382784+00:00"},{"alias_kind":"pith_short_16","alias_value":"6GQ7DDUBEQIA7ZQ6","created_at":"2026-07-05T07:35:46.382784+00:00"},{"alias_kind":"pith_short_8","alias_value":"6GQ7DDUB","created_at":"2026-07-05T07:35:46.382784+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.06478","citing_title":"Selected Results on Variable Stars Observed by TESS","ref_index":76,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX","json":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX.json","graph_json":"https://pith.science/api/pith-number/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/graph.json","events_json":"https://pith.science/api/pith-number/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/events.json","paper":"https://pith.science/paper/6GQ7DDUB"},"agent_actions":{"view_html":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX","download_json":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX.json","view_paper":"https://pith.science/paper/6GQ7DDUB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2401.11134&json=true","fetch_graph":"https://pith.science/api/pith-number/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/graph.json","fetch_events":"https://pith.science/api/pith-number/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/action/storage_attestation","attest_author":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/action/author_attestation","sign_citation":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/action/citation_signature","submit_replication":"https://pith.science/pith/6GQ7DDUBEQIA7ZQ6RRBXFIO6WX/action/replication_record"}},"created_at":"2026-07-05T07:35:46.382784+00:00","updated_at":"2026-07-05T07:35:46.382784+00:00"}