{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:QSLVZQXQG3D3BZCIUFQS5Y3YPJ","short_pith_number":"pith:QSLVZQXQ","schema_version":"1.0","canonical_sha256":"84975cc2f036c7b0e448a1612ee3787a5fa25bec76e161250ee47be03097e2a8","source":{"kind":"arxiv","id":"1001.2796","version":1},"attestation_state":"computed","paper":{"title":"Li I and K I Scatter in Cool Pleiades Dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"J.R. King, L.M. Hobbs, M.H. Pinsonneault, S.C. Schuler","submitted_at":"2010-01-16T00:11:20Z","abstract_excerpt":"We utilize high-resolution (R~60,000), high S/N (~100) spectroscopy of 17 cool Pleiades dwarfs to examine the confounding star-to-star scatter in the 6707 Li I line strengths in this young cluster. Our Pleiads, selected for their small projected rotational velocity and modest chromospheric emission, evince substantial scatter in the linestrengths of 6707 Li I feature that is absent in the 7699 K I resonance line. The Li I scatter is not correlated with that in the high-excitation 7774 O I feature, and the magnitude of the former is greater than the latter despite the larger temperature sensiti"},"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":"1001.2796","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-01-16T00:11:20Z","cross_cats_sorted":[],"title_canon_sha256":"c8744588b6fac98ee9abe76ab89c6ef6d14c8a31da0916eee07fe18e980c7a5b","abstract_canon_sha256":"5c1695b2ce6111abeb8aaafda7a130a79da4e4850506e395c2892eb4620f61f4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:09:43.531497Z","signature_b64":"I8gO2OoDGb4nOeSZfvVhT6c3M3LhYglV3KINw/SUbTvPFY0SJL9IioU6OtkiCkEVl96eRvNmXj/5aJJxwueHCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"84975cc2f036c7b0e448a1612ee3787a5fa25bec76e161250ee47be03097e2a8","last_reissued_at":"2026-05-18T02:09:43.530643Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:09:43.530643Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Li I and K I Scatter in Cool Pleiades Dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"J.R. King, L.M. Hobbs, M.H. Pinsonneault, S.C. Schuler","submitted_at":"2010-01-16T00:11:20Z","abstract_excerpt":"We utilize high-resolution (R~60,000), high S/N (~100) spectroscopy of 17 cool Pleiades dwarfs to examine the confounding star-to-star scatter in the 6707 Li I line strengths in this young cluster. Our Pleiads, selected for their small projected rotational velocity and modest chromospheric emission, evince substantial scatter in the linestrengths of 6707 Li I feature that is absent in the 7699 K I resonance line. The Li I scatter is not correlated with that in the high-excitation 7774 O I feature, and the magnitude of the former is greater than the latter despite the larger temperature sensiti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1001.2796","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":"1001.2796","created_at":"2026-05-18T02:09:43.530788+00:00"},{"alias_kind":"arxiv_version","alias_value":"1001.2796v1","created_at":"2026-05-18T02:09:43.530788+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1001.2796","created_at":"2026-05-18T02:09:43.530788+00:00"},{"alias_kind":"pith_short_12","alias_value":"QSLVZQXQG3D3","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_16","alias_value":"QSLVZQXQG3D3BZCI","created_at":"2026-05-18T12:26:12.377268+00:00"},{"alias_kind":"pith_short_8","alias_value":"QSLVZQXQ","created_at":"2026-05-18T12:26:12.377268+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/QSLVZQXQG3D3BZCIUFQS5Y3YPJ","json":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ.json","graph_json":"https://pith.science/api/pith-number/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/graph.json","events_json":"https://pith.science/api/pith-number/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/events.json","paper":"https://pith.science/paper/QSLVZQXQ"},"agent_actions":{"view_html":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ","download_json":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ.json","view_paper":"https://pith.science/paper/QSLVZQXQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1001.2796&json=true","fetch_graph":"https://pith.science/api/pith-number/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/graph.json","fetch_events":"https://pith.science/api/pith-number/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/action/storage_attestation","attest_author":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/action/author_attestation","sign_citation":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/action/citation_signature","submit_replication":"https://pith.science/pith/QSLVZQXQG3D3BZCIUFQS5Y3YPJ/action/replication_record"}},"created_at":"2026-05-18T02:09:43.530788+00:00","updated_at":"2026-05-18T02:09:43.530788+00:00"}