{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:OF7BEW5LLW2BDZXO2H6EWZEJDM","short_pith_number":"pith:OF7BEW5L","schema_version":"1.0","canonical_sha256":"717e125bab5db411e6eed1fc4b64891b3c9f8cbbf7c17ca39e6de281184f5d59","source":{"kind":"arxiv","id":"1811.06594","version":1},"attestation_state":"computed","paper":{"title":"Searching for the Origin of Flares in M dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Gavin Ramsay, John G. Doyle, Lauren Doyle","submitted_at":"2018-11-15T21:09:19Z","abstract_excerpt":"We present an overview of K2 short cadence observations for 34 M dwarfs observed in Campaigns 1 - 9 which have spectral types between M0 - L1. All of the stars in our sample showed flares with the most energetic reaching $3\\times10^{34}$ ergs. As previous studies have found, we find rapidly rotating stars tend to show more flares, with evidence for a decline in activity in stars with rotation periods longer than approximately 10 days. We determined the rotational phase of each flare and performed a simple statistical test on our sample to determine whether the phase distribution of the flares "},"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":"1811.06594","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-11-15T21:09:19Z","cross_cats_sorted":[],"title_canon_sha256":"08a09a7e6db691097b3846adc02501dcdb74a9da0192e51d7727faa6ebded29e","abstract_canon_sha256":"f1649544b74403c894d1b1113c92d8574911557e49a61e6484256912719c2b97"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:04.274571Z","signature_b64":"7kHkn43/M+E0mfqTiU3IssDxnSLsDzYZr1AsYc3dGcVdDfRLAFpUgNTr5RKJzu3CqEQrzye2YwvP1l+omfHJDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"717e125bab5db411e6eed1fc4b64891b3c9f8cbbf7c17ca39e6de281184f5d59","last_reissued_at":"2026-05-17T23:52:04.273936Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:04.273936Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Searching for the Origin of Flares in M dwarfs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Gavin Ramsay, John G. Doyle, Lauren Doyle","submitted_at":"2018-11-15T21:09:19Z","abstract_excerpt":"We present an overview of K2 short cadence observations for 34 M dwarfs observed in Campaigns 1 - 9 which have spectral types between M0 - L1. All of the stars in our sample showed flares with the most energetic reaching $3\\times10^{34}$ ergs. As previous studies have found, we find rapidly rotating stars tend to show more flares, with evidence for a decline in activity in stars with rotation periods longer than approximately 10 days. We determined the rotational phase of each flare and performed a simple statistical test on our sample to determine whether the phase distribution of the flares "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.06594","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":"1811.06594","created_at":"2026-05-17T23:52:04.274014+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.06594v1","created_at":"2026-05-17T23:52:04.274014+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.06594","created_at":"2026-05-17T23:52:04.274014+00:00"},{"alias_kind":"pith_short_12","alias_value":"OF7BEW5LLW2B","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_16","alias_value":"OF7BEW5LLW2BDZXO","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_8","alias_value":"OF7BEW5L","created_at":"2026-05-18T12:32:43.782077+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/OF7BEW5LLW2BDZXO2H6EWZEJDM","json":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM.json","graph_json":"https://pith.science/api/pith-number/OF7BEW5LLW2BDZXO2H6EWZEJDM/graph.json","events_json":"https://pith.science/api/pith-number/OF7BEW5LLW2BDZXO2H6EWZEJDM/events.json","paper":"https://pith.science/paper/OF7BEW5L"},"agent_actions":{"view_html":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM","download_json":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM.json","view_paper":"https://pith.science/paper/OF7BEW5L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.06594&json=true","fetch_graph":"https://pith.science/api/pith-number/OF7BEW5LLW2BDZXO2H6EWZEJDM/graph.json","fetch_events":"https://pith.science/api/pith-number/OF7BEW5LLW2BDZXO2H6EWZEJDM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM/action/storage_attestation","attest_author":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM/action/author_attestation","sign_citation":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM/action/citation_signature","submit_replication":"https://pith.science/pith/OF7BEW5LLW2BDZXO2H6EWZEJDM/action/replication_record"}},"created_at":"2026-05-17T23:52:04.274014+00:00","updated_at":"2026-05-17T23:52:04.274014+00:00"}