{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:OMQ24V7MFHM6LRKALM6O455L2J","short_pith_number":"pith:OMQ24V7M","schema_version":"1.0","canonical_sha256":"7321ae57ec29d9e5c5405b3cee77abd27c6fac6df6bf9eb004a490f9ee438360","source":{"kind":"arxiv","id":"1309.1012","version":1},"attestation_state":"computed","paper":{"title":"Variability of M giant stars based on Kepler photometry: general characteristics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. B\\'odi, A. Derekas, A. E. Simon, B. Bellamy, D. Compton, D. Huber, D. Stello, E. B\\'anyai, Gy. M. Szab\\'o, I. Cs\\'anyi, J. Dorval, J. M. Benk\\H{o}, J. R. Callingham, K. Szatm\\'ary, L. L. Kiss, O. Shrier, R. Szab\\'o, T. R. Bedding","submitted_at":"2013-09-04T12:53:03Z","abstract_excerpt":"M giants are among the longest-period pulsating stars which is why their studies were traditionally restricted to analyses of low-precision visual observations, and more recently, accurate ground-based data. Here we present an overview of M giant variability on a wide range of time-scales (hours to years), based on analysis of thirteen quarters of Kepler long-cadence observations (one point per every 29.4 minutes), with a total time-span of over 1000 days. About two-thirds of the sample stars have been selected from the ASAS-North survey of the Kepler field, with the rest supplemented from a r"},"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":"1309.1012","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-09-04T12:53:03Z","cross_cats_sorted":[],"title_canon_sha256":"d6d5bcfb73420f8a3ada73b6650ac12732e88f5b5a7d42373bfbddb94fcdcbc2","abstract_canon_sha256":"b7696e7330f51943daa5f1d17b34d04685136785c1c29121eafbfc2e5b1288ac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:47:49.884244Z","signature_b64":"tj0R0AYiRs7nr5sHTroCAHsvmaBGiI1D2oOswdz3D5BBaCalS+KKfmGut/VrmtoIgJbtp7LycrEa+mRffuvHAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7321ae57ec29d9e5c5405b3cee77abd27c6fac6df6bf9eb004a490f9ee438360","last_reissued_at":"2026-05-18T01:47:49.883840Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:47:49.883840Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Variability of M giant stars based on Kepler photometry: general characteristics","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. B\\'odi, A. Derekas, A. E. Simon, B. Bellamy, D. Compton, D. Huber, D. Stello, E. B\\'anyai, Gy. M. Szab\\'o, I. Cs\\'anyi, J. Dorval, J. M. Benk\\H{o}, J. R. Callingham, K. Szatm\\'ary, L. L. Kiss, O. Shrier, R. Szab\\'o, T. R. Bedding","submitted_at":"2013-09-04T12:53:03Z","abstract_excerpt":"M giants are among the longest-period pulsating stars which is why their studies were traditionally restricted to analyses of low-precision visual observations, and more recently, accurate ground-based data. Here we present an overview of M giant variability on a wide range of time-scales (hours to years), based on analysis of thirteen quarters of Kepler long-cadence observations (one point per every 29.4 minutes), with a total time-span of over 1000 days. About two-thirds of the sample stars have been selected from the ASAS-North survey of the Kepler field, with the rest supplemented from a r"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.1012","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":"1309.1012","created_at":"2026-05-18T01:47:49.883897+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.1012v1","created_at":"2026-05-18T01:47:49.883897+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.1012","created_at":"2026-05-18T01:47:49.883897+00:00"},{"alias_kind":"pith_short_12","alias_value":"OMQ24V7MFHM6","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_16","alias_value":"OMQ24V7MFHM6LRKA","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_8","alias_value":"OMQ24V7M","created_at":"2026-05-18T12:27:54.935989+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/OMQ24V7MFHM6LRKALM6O455L2J","json":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J.json","graph_json":"https://pith.science/api/pith-number/OMQ24V7MFHM6LRKALM6O455L2J/graph.json","events_json":"https://pith.science/api/pith-number/OMQ24V7MFHM6LRKALM6O455L2J/events.json","paper":"https://pith.science/paper/OMQ24V7M"},"agent_actions":{"view_html":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J","download_json":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J.json","view_paper":"https://pith.science/paper/OMQ24V7M","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.1012&json=true","fetch_graph":"https://pith.science/api/pith-number/OMQ24V7MFHM6LRKALM6O455L2J/graph.json","fetch_events":"https://pith.science/api/pith-number/OMQ24V7MFHM6LRKALM6O455L2J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J/action/storage_attestation","attest_author":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J/action/author_attestation","sign_citation":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J/action/citation_signature","submit_replication":"https://pith.science/pith/OMQ24V7MFHM6LRKALM6O455L2J/action/replication_record"}},"created_at":"2026-05-18T01:47:49.883897+00:00","updated_at":"2026-05-18T01:47:49.883897+00:00"}