{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:FLODQRGLCKEL2CWHK4UZL3QNGJ","short_pith_number":"pith:FLODQRGL","schema_version":"1.0","canonical_sha256":"2adc3844cb1288bd0ac7572995ee0d3241932bc2a0dd656a1b345a465877da66","source":{"kind":"arxiv","id":"1610.08811","version":1},"attestation_state":"computed","paper":{"title":"CSI 2264: Investigating rotation and its connection with disk accretion in the young open cluster NGC 2264","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. M. Cody, A. P. Sousa, E. Flaccomio, G. Micela, J. Bouvier, J. R. Stauffer, L. A. Hillenbrand, L. M. Rebull, L. Venuti, S. H. P. Alencar","submitted_at":"2016-10-27T14:44:02Z","abstract_excerpt":"The low spin rates measured for solar-type stars at an age of a few Myr (~10% of the break-up velocity) indicate that some mechanism of angular momentum regulation must be at play in the early pre-main sequence. We characterize the rotation properties for members of the region NGC 2264 (~3 Myr), and investigate the accretion-rotation connection at an age where about 50% of the stars have already lost their disks. We examined a sample of 500 cluster members whose photometric variations were monitored in the optical for 38 consecutive days with CoRoT. Light curves were analyzed for periodicity u"},"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":"1610.08811","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2016-10-27T14:44:02Z","cross_cats_sorted":[],"title_canon_sha256":"80b77025e47175a7d89fd64bb82b1a1853418afc3965093f32855b8830f22dfd","abstract_canon_sha256":"cb1090e084735a001b02b29b7f71280efe8b713c31f0935b8e15ac7ad59d798c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:18.418678Z","signature_b64":"x7FXwyrx7XNoETzS3bqonqCglWiEZRrjdZzP1hK+tJCGABuo8MZ+rnuZAq/Babi7NXJSDrVZETEECbeshWkbBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2adc3844cb1288bd0ac7572995ee0d3241932bc2a0dd656a1b345a465877da66","last_reissued_at":"2026-05-18T00:50:18.418121Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:18.418121Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CSI 2264: Investigating rotation and its connection with disk accretion in the young open cluster NGC 2264","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. M. Cody, A. P. Sousa, E. Flaccomio, G. Micela, J. Bouvier, J. R. Stauffer, L. A. Hillenbrand, L. M. Rebull, L. Venuti, S. H. P. Alencar","submitted_at":"2016-10-27T14:44:02Z","abstract_excerpt":"The low spin rates measured for solar-type stars at an age of a few Myr (~10% of the break-up velocity) indicate that some mechanism of angular momentum regulation must be at play in the early pre-main sequence. We characterize the rotation properties for members of the region NGC 2264 (~3 Myr), and investigate the accretion-rotation connection at an age where about 50% of the stars have already lost their disks. We examined a sample of 500 cluster members whose photometric variations were monitored in the optical for 38 consecutive days with CoRoT. Light curves were analyzed for periodicity u"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.08811","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":"1610.08811","created_at":"2026-05-18T00:50:18.418201+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.08811v1","created_at":"2026-05-18T00:50:18.418201+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.08811","created_at":"2026-05-18T00:50:18.418201+00:00"},{"alias_kind":"pith_short_12","alias_value":"FLODQRGLCKEL","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_16","alias_value":"FLODQRGLCKEL2CWH","created_at":"2026-05-18T12:30:15.759754+00:00"},{"alias_kind":"pith_short_8","alias_value":"FLODQRGL","created_at":"2026-05-18T12:30:15.759754+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/FLODQRGLCKEL2CWHK4UZL3QNGJ","json":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ.json","graph_json":"https://pith.science/api/pith-number/FLODQRGLCKEL2CWHK4UZL3QNGJ/graph.json","events_json":"https://pith.science/api/pith-number/FLODQRGLCKEL2CWHK4UZL3QNGJ/events.json","paper":"https://pith.science/paper/FLODQRGL"},"agent_actions":{"view_html":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ","download_json":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ.json","view_paper":"https://pith.science/paper/FLODQRGL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.08811&json=true","fetch_graph":"https://pith.science/api/pith-number/FLODQRGLCKEL2CWHK4UZL3QNGJ/graph.json","fetch_events":"https://pith.science/api/pith-number/FLODQRGLCKEL2CWHK4UZL3QNGJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ/action/storage_attestation","attest_author":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ/action/author_attestation","sign_citation":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ/action/citation_signature","submit_replication":"https://pith.science/pith/FLODQRGLCKEL2CWHK4UZL3QNGJ/action/replication_record"}},"created_at":"2026-05-18T00:50:18.418201+00:00","updated_at":"2026-05-18T00:50:18.418201+00:00"}