{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:6YNFRUFRN4Z6ALPZLEPT23MVY6","short_pith_number":"pith:6YNFRUFR","schema_version":"1.0","canonical_sha256":"f61a58d0b16f33e02df9591f3d6d95c7b590dfd6b31468831b9b2cd71d425f48","source":{"kind":"arxiv","id":"1901.01974","version":3},"attestation_state":"computed","paper":{"title":"Revisiting the Long-Period Transiting Planets from Kepler","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Miranda K. Herman, Wei Zhu, Yanqin Wu","submitted_at":"2019-01-07T18:59:53Z","abstract_excerpt":"Currently, we have only limited means to probe the presence of planets at large orbital separations. Foreman-Mackey et al. searched for long-period transiting planets in the Kepler light curves using an automated pipeline. Here, we apply their pipeline, with minor modifications, to a larger sample and use updated stellar parameters from Gaia DR2. The latter boosts the stellar radii for most of the planet candidates found by FM16, invalidating a number of them as false positives. We identify 15 candidates, including two new ones. All have sizes from 0.3 to 1 $R_{\\rm J}$, and all but two have pe"},"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":"1901.01974","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2019-01-07T18:59:53Z","cross_cats_sorted":[],"title_canon_sha256":"c837949acd2ae0cb8e81f0c313ec879fca62e246302ea7fee6c97279e9b4c49f","abstract_canon_sha256":"7d9a96d79e22d11bdb4f723db2c5328b48d5800cc18db48376758b02903268a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:40:33.735449Z","signature_b64":"Hu5qTiBL4jZPj/KGbF7HDglsV4su8rzI6v2CbSzpEL9pA73apOkbdfZ+F1Cr5uXzVMfP/CkzYqyp2HJrlQr0DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f61a58d0b16f33e02df9591f3d6d95c7b590dfd6b31468831b9b2cd71d425f48","last_reissued_at":"2026-05-17T23:40:33.734785Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:40:33.734785Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revisiting the Long-Period Transiting Planets from Kepler","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Miranda K. Herman, Wei Zhu, Yanqin Wu","submitted_at":"2019-01-07T18:59:53Z","abstract_excerpt":"Currently, we have only limited means to probe the presence of planets at large orbital separations. Foreman-Mackey et al. searched for long-period transiting planets in the Kepler light curves using an automated pipeline. Here, we apply their pipeline, with minor modifications, to a larger sample and use updated stellar parameters from Gaia DR2. The latter boosts the stellar radii for most of the planet candidates found by FM16, invalidating a number of them as false positives. We identify 15 candidates, including two new ones. All have sizes from 0.3 to 1 $R_{\\rm J}$, and all but two have pe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.01974","kind":"arxiv","version":3},"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":"1901.01974","created_at":"2026-05-17T23:40:33.734863+00:00"},{"alias_kind":"arxiv_version","alias_value":"1901.01974v3","created_at":"2026-05-17T23:40:33.734863+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1901.01974","created_at":"2026-05-17T23:40:33.734863+00:00"},{"alias_kind":"pith_short_12","alias_value":"6YNFRUFRN4Z6","created_at":"2026-05-18T12:33:10.108867+00:00"},{"alias_kind":"pith_short_16","alias_value":"6YNFRUFRN4Z6ALPZ","created_at":"2026-05-18T12:33:10.108867+00:00"},{"alias_kind":"pith_short_8","alias_value":"6YNFRUFR","created_at":"2026-05-18T12:33:10.108867+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/6YNFRUFRN4Z6ALPZLEPT23MVY6","json":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6.json","graph_json":"https://pith.science/api/pith-number/6YNFRUFRN4Z6ALPZLEPT23MVY6/graph.json","events_json":"https://pith.science/api/pith-number/6YNFRUFRN4Z6ALPZLEPT23MVY6/events.json","paper":"https://pith.science/paper/6YNFRUFR"},"agent_actions":{"view_html":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6","download_json":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6.json","view_paper":"https://pith.science/paper/6YNFRUFR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1901.01974&json=true","fetch_graph":"https://pith.science/api/pith-number/6YNFRUFRN4Z6ALPZLEPT23MVY6/graph.json","fetch_events":"https://pith.science/api/pith-number/6YNFRUFRN4Z6ALPZLEPT23MVY6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6/action/storage_attestation","attest_author":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6/action/author_attestation","sign_citation":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6/action/citation_signature","submit_replication":"https://pith.science/pith/6YNFRUFRN4Z6ALPZLEPT23MVY6/action/replication_record"}},"created_at":"2026-05-17T23:40:33.734863+00:00","updated_at":"2026-05-17T23:40:33.734863+00:00"}