{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:F32EYSG5GDDG4MO2G4BSZMYBR2","short_pith_number":"pith:F32EYSG5","schema_version":"1.0","canonical_sha256":"2ef44c48dd30c66e31da37032cb3018e9fbe297f2bd06fc93a00cda93e1fb5cc","source":{"kind":"arxiv","id":"2412.10508","version":1},"attestation_state":"computed","paper":{"title":"MOCKA -- A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"A. Bodi, A. Tkachenko, C. Aerts, D. J. Fritzewski, D. M. Bowman, D. Seynaeve, E. Plachy, G. Li, J. De Ridder, L. W. IJspeert, M. G. Pedersen, M. Uzundag, M. Vanrespaille, N. Jannsen, P. Royer, S. Aigrain, T. Van Reeth","submitted_at":"2024-12-13T19:00:46Z","abstract_excerpt":"With ESA's PLATO space mission set for launch in December 2026, a new photometric legacy and a future of new scientific discoveries await. In this work we investigate PLATO's potential for observing pulsating stars across the Hertzsprung-Russell diagram as part of the PLATO Complimentary Science program (PLATO-CS). Specifically, a PLATO mock asteroseismic catalogue (MOCKA) of intermediate to massive stars is presented as a benchmark to highlight the asteroseismic yield of PLATO-CS in a quantitative way. MOCKA includes simulations of $\\beta$~Cephei, slowly pulsating B (SPB), $\\delta$~Scuti, $\\g"},"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":"2412.10508","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.SR","submitted_at":"2024-12-13T19:00:46Z","cross_cats_sorted":["astro-ph.EP","astro-ph.GA","astro-ph.IM"],"title_canon_sha256":"d0b90b9ec9f29cefb29ca0728edbf8e49de27bc0e0e7daf08619b427509eae49","abstract_canon_sha256":"9567dc5d9a275c60b4ddb6880e581f92b0764f89570e13ab75c4b5e2913133fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:12:51.047059Z","signature_b64":"bGTp2dhHWM/OC5+HObXswS8appcTJurmBeO3kV3QFqSRwgGT5Vt/+zmNNtcIfy5+DrihwwMoy07ilXTcRYz+DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2ef44c48dd30c66e31da37032cb3018e9fbe297f2bd06fc93a00cda93e1fb5cc","last_reissued_at":"2026-07-05T10:12:51.046547Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:12:51.046547Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"MOCKA -- A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"A. Bodi, A. Tkachenko, C. Aerts, D. J. Fritzewski, D. M. Bowman, D. Seynaeve, E. Plachy, G. Li, J. De Ridder, L. W. IJspeert, M. G. Pedersen, M. Uzundag, M. Vanrespaille, N. Jannsen, P. Royer, S. Aigrain, T. Van Reeth","submitted_at":"2024-12-13T19:00:46Z","abstract_excerpt":"With ESA's PLATO space mission set for launch in December 2026, a new photometric legacy and a future of new scientific discoveries await. In this work we investigate PLATO's potential for observing pulsating stars across the Hertzsprung-Russell diagram as part of the PLATO Complimentary Science program (PLATO-CS). Specifically, a PLATO mock asteroseismic catalogue (MOCKA) of intermediate to massive stars is presented as a benchmark to highlight the asteroseismic yield of PLATO-CS in a quantitative way. MOCKA includes simulations of $\\beta$~Cephei, slowly pulsating B (SPB), $\\delta$~Scuti, $\\g"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.10508","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/2412.10508/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":"2412.10508","created_at":"2026-07-05T10:12:51.046620+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.10508v1","created_at":"2026-07-05T10:12:51.046620+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.10508","created_at":"2026-07-05T10:12:51.046620+00:00"},{"alias_kind":"pith_short_12","alias_value":"F32EYSG5GDDG","created_at":"2026-07-05T10:12:51.046620+00:00"},{"alias_kind":"pith_short_16","alias_value":"F32EYSG5GDDG4MO2","created_at":"2026-07-05T10:12:51.046620+00:00"},{"alias_kind":"pith_short_8","alias_value":"F32EYSG5","created_at":"2026-07-05T10:12:51.046620+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.10834","citing_title":"Asteroseismic forward modelling of 36 $\\beta$ Cep pulsators and inferences on their internal differential rotation","ref_index":77,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2","json":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2.json","graph_json":"https://pith.science/api/pith-number/F32EYSG5GDDG4MO2G4BSZMYBR2/graph.json","events_json":"https://pith.science/api/pith-number/F32EYSG5GDDG4MO2G4BSZMYBR2/events.json","paper":"https://pith.science/paper/F32EYSG5"},"agent_actions":{"view_html":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2","download_json":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2.json","view_paper":"https://pith.science/paper/F32EYSG5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.10508&json=true","fetch_graph":"https://pith.science/api/pith-number/F32EYSG5GDDG4MO2G4BSZMYBR2/graph.json","fetch_events":"https://pith.science/api/pith-number/F32EYSG5GDDG4MO2G4BSZMYBR2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2/action/storage_attestation","attest_author":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2/action/author_attestation","sign_citation":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2/action/citation_signature","submit_replication":"https://pith.science/pith/F32EYSG5GDDG4MO2G4BSZMYBR2/action/replication_record"}},"created_at":"2026-07-05T10:12:51.046620+00:00","updated_at":"2026-07-05T10:12:51.046620+00:00"}