{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:ZCCD4BC6F7E4WDJAUTBUKI3VVE","short_pith_number":"pith:ZCCD4BC6","schema_version":"1.0","canonical_sha256":"c8843e045e2fc9cb0d20a4c3452375a938d8ccecc8da63e124f408c2f301d0a6","source":{"kind":"arxiv","id":"1806.06075","version":2},"attestation_state":"computed","paper":{"title":"Stability of exomoons around the Kepler transiting circumbinary planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adrian S. Hamers, Javier Roa, Maxwell X. Cai, Nathan Leigh","submitted_at":"2018-06-15T18:00:07Z","abstract_excerpt":"The Kepler mission has detected a number of transiting circumbinary planets (CBPs). Although currently not detected, exomoons could be orbiting some of these CBPs, and they might be suitable for harboring life. A necessary condition for the existence of such exomoons is their long-term dynamical stability. Here, we investigate the stability of exomoons around the Kepler CBPs using numerical $N$-body integrations. We determine regions of stability and obtain stability maps in the (a_m,i_pm) plane, where a_m is the initial exolunar semimajor axis with respect to the CBP, and i_pm is the initial "},"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":"1806.06075","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2018-06-15T18:00:07Z","cross_cats_sorted":[],"title_canon_sha256":"cf0aea794b85fbc2d867dd9ff092ba76d3fb0b8193f0ab6c5286fed47510ba69","abstract_canon_sha256":"53d716ff7c900d4509fa50d0f80681795960624639a7d42b449f07cb808ed41c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:08:14.667329Z","signature_b64":"et1Cm0EFMh967wRtxwU1sbfxkHEkMXsGmWTXz7hoC6oDI0a/j0O0ydQoQqYu1Zmo5rxecgrD6XEtDHQmaqpzAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c8843e045e2fc9cb0d20a4c3452375a938d8ccecc8da63e124f408c2f301d0a6","last_reissued_at":"2026-05-18T00:08:14.666945Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:08:14.666945Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stability of exomoons around the Kepler transiting circumbinary planets","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Adrian S. Hamers, Javier Roa, Maxwell X. Cai, Nathan Leigh","submitted_at":"2018-06-15T18:00:07Z","abstract_excerpt":"The Kepler mission has detected a number of transiting circumbinary planets (CBPs). Although currently not detected, exomoons could be orbiting some of these CBPs, and they might be suitable for harboring life. A necessary condition for the existence of such exomoons is their long-term dynamical stability. Here, we investigate the stability of exomoons around the Kepler CBPs using numerical $N$-body integrations. We determine regions of stability and obtain stability maps in the (a_m,i_pm) plane, where a_m is the initial exolunar semimajor axis with respect to the CBP, and i_pm is the initial "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.06075","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":""},"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":"1806.06075","created_at":"2026-05-18T00:08:14.667001+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.06075v2","created_at":"2026-05-18T00:08:14.667001+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.06075","created_at":"2026-05-18T00:08:14.667001+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZCCD4BC6F7E4","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZCCD4BC6F7E4WDJA","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZCCD4BC6","created_at":"2026-05-18T12:33:04.347982+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/ZCCD4BC6F7E4WDJAUTBUKI3VVE","json":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE.json","graph_json":"https://pith.science/api/pith-number/ZCCD4BC6F7E4WDJAUTBUKI3VVE/graph.json","events_json":"https://pith.science/api/pith-number/ZCCD4BC6F7E4WDJAUTBUKI3VVE/events.json","paper":"https://pith.science/paper/ZCCD4BC6"},"agent_actions":{"view_html":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE","download_json":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE.json","view_paper":"https://pith.science/paper/ZCCD4BC6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.06075&json=true","fetch_graph":"https://pith.science/api/pith-number/ZCCD4BC6F7E4WDJAUTBUKI3VVE/graph.json","fetch_events":"https://pith.science/api/pith-number/ZCCD4BC6F7E4WDJAUTBUKI3VVE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE/action/storage_attestation","attest_author":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE/action/author_attestation","sign_citation":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE/action/citation_signature","submit_replication":"https://pith.science/pith/ZCCD4BC6F7E4WDJAUTBUKI3VVE/action/replication_record"}},"created_at":"2026-05-18T00:08:14.667001+00:00","updated_at":"2026-05-18T00:08:14.667001+00:00"}