{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:TMK5PCS4ZXXECTRJL4SLFXFIXY","short_pith_number":"pith:TMK5PCS4","schema_version":"1.0","canonical_sha256":"9b15d78a5ccdee414e295f24b2dca8be300ced203ed1bcffb4176cd232914f03","source":{"kind":"arxiv","id":"2407.15917","version":2},"attestation_state":"computed","paper":{"title":"Exoplanets Across Galactic Stellar Populations with PLATO: Estimating Exoplanet Yields Around FGK Stars for the Thin Disk, Thick Disk and Stellar Halo","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Akshara Viswanathan, Christopher Boettner, Pratika Dayal","submitted_at":"2024-07-22T18:00:00Z","abstract_excerpt":"This study aims to assess the potential of the upcoming PLATO mission to investigate exoplanet populations around stars in diverse Galactic environments, specifically focusing on the Milky Way thin disk, thick disk, and stellar halo. We aim to quantify PLATOs ability to detect planets in each environment and determine how these observations could constrain planet formation models. Beginning from the all-sky PLATO Input Catalog, we kinematically classify the 2.4 million FGK stars into their respective Galactic components. For the sub-sample of stars in the long-observation LOPS2 and LOPN1 PLATO"},"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":"2407.15917","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2024-07-22T18:00:00Z","cross_cats_sorted":["astro-ph.GA","astro-ph.SR"],"title_canon_sha256":"94bfc7d35e85199f77a41c22c6cad8068dbe0e2b9fb3e5d2b721179683ae3945","abstract_canon_sha256":"2fea9d448ed23719fc940b55dace6c72da427682902a05532ae76c18b9213b00"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:34:16.935518Z","signature_b64":"xAnB2KpsLvOGGFJwJEEQFmjaXzvFDAB5gnG1jwssetlwEVeJK0j6xmcdQzeusYB0JWoK5uJKhsdU6/DANAV+Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b15d78a5ccdee414e295f24b2dca8be300ced203ed1bcffb4176cd232914f03","last_reissued_at":"2026-07-05T09:34:16.935104Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:34:16.935104Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exoplanets Across Galactic Stellar Populations with PLATO: Estimating Exoplanet Yields Around FGK Stars for the Thin Disk, Thick Disk and Stellar Halo","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Akshara Viswanathan, Christopher Boettner, Pratika Dayal","submitted_at":"2024-07-22T18:00:00Z","abstract_excerpt":"This study aims to assess the potential of the upcoming PLATO mission to investigate exoplanet populations around stars in diverse Galactic environments, specifically focusing on the Milky Way thin disk, thick disk, and stellar halo. We aim to quantify PLATOs ability to detect planets in each environment and determine how these observations could constrain planet formation models. Beginning from the all-sky PLATO Input Catalog, we kinematically classify the 2.4 million FGK stars into their respective Galactic components. For the sub-sample of stars in the long-observation LOPS2 and LOPN1 PLATO"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.15917","kind":"arxiv","version":2},"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/2407.15917/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":"2407.15917","created_at":"2026-07-05T09:34:16.935167+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.15917v2","created_at":"2026-07-05T09:34:16.935167+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.15917","created_at":"2026-07-05T09:34:16.935167+00:00"},{"alias_kind":"pith_short_12","alias_value":"TMK5PCS4ZXXE","created_at":"2026-07-05T09:34:16.935167+00:00"},{"alias_kind":"pith_short_16","alias_value":"TMK5PCS4ZXXECTRJ","created_at":"2026-07-05T09:34:16.935167+00:00"},{"alias_kind":"pith_short_8","alias_value":"TMK5PCS4","created_at":"2026-07-05T09:34:16.935167+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.09656","citing_title":"HD 148797: A bright F-type star with two moderate-period low-density sub-Jovian planets. Compact multi-planet architectures are common in the Neptunian savanna","ref_index":186,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY","json":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY.json","graph_json":"https://pith.science/api/pith-number/TMK5PCS4ZXXECTRJL4SLFXFIXY/graph.json","events_json":"https://pith.science/api/pith-number/TMK5PCS4ZXXECTRJL4SLFXFIXY/events.json","paper":"https://pith.science/paper/TMK5PCS4"},"agent_actions":{"view_html":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY","download_json":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY.json","view_paper":"https://pith.science/paper/TMK5PCS4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.15917&json=true","fetch_graph":"https://pith.science/api/pith-number/TMK5PCS4ZXXECTRJL4SLFXFIXY/graph.json","fetch_events":"https://pith.science/api/pith-number/TMK5PCS4ZXXECTRJL4SLFXFIXY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY/action/storage_attestation","attest_author":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY/action/author_attestation","sign_citation":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY/action/citation_signature","submit_replication":"https://pith.science/pith/TMK5PCS4ZXXECTRJL4SLFXFIXY/action/replication_record"}},"created_at":"2026-07-05T09:34:16.935167+00:00","updated_at":"2026-07-05T09:34:16.935167+00:00"}