{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:CI5WSAPJMHKXLAHMYPVFCE6PNW","short_pith_number":"pith:CI5WSAPJ","schema_version":"1.0","canonical_sha256":"123b6901e961d57580ecc3ea5113cf6da1440a728841c81e41556bc86531075b","source":{"kind":"arxiv","id":"1302.6244","version":2},"attestation_state":"computed","paper":{"title":"Giant planets orbiting metal-rich stars show signatures of planet-planet interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Rebekah I. Dawson, Ruth A. Murray-Clay","submitted_at":"2013-02-25T21:00:56Z","abstract_excerpt":"Gas giants orbiting interior to the ice line are thought to have been displaced from their formation locations by processes that remain debated. Here we uncover several new metallicity trends, which together may indicate that two competing mechanisms deliver close-in giant planets: gentle disk migration, operating in environments with a range of metallicities, and violent planet-planet gravitational interactions, primarily triggered in metal-rich systems in which multiple giant planets can form. First, we show with 99.1% confidence that giant planets with semi-major axes between 0.1 and 1 AU o"},"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":"1302.6244","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2013-02-25T21:00:56Z","cross_cats_sorted":[],"title_canon_sha256":"2e98f9d2b804b824bfb7698cc9786a302cbf593748b7aa4c2b8c9c23ab09300b","abstract_canon_sha256":"c4ae359520329826788bf6421a62615efb18941388a95c921c7ff4dcdbeba82f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:19:13.137247Z","signature_b64":"mn5Nxs9TAVWQMzwpcCb5TxxtEIE3ICYRKTDpYb+cQ4KHB1F0Cwi1O8HEEDD9zL7aFAUTlszE+uAXWRUidES2Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"123b6901e961d57580ecc3ea5113cf6da1440a728841c81e41556bc86531075b","last_reissued_at":"2026-05-18T03:19:13.136719Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:19:13.136719Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Giant planets orbiting metal-rich stars show signatures of planet-planet interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Rebekah I. Dawson, Ruth A. Murray-Clay","submitted_at":"2013-02-25T21:00:56Z","abstract_excerpt":"Gas giants orbiting interior to the ice line are thought to have been displaced from their formation locations by processes that remain debated. Here we uncover several new metallicity trends, which together may indicate that two competing mechanisms deliver close-in giant planets: gentle disk migration, operating in environments with a range of metallicities, and violent planet-planet gravitational interactions, primarily triggered in metal-rich systems in which multiple giant planets can form. First, we show with 99.1% confidence that giant planets with semi-major axes between 0.1 and 1 AU o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1302.6244","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":"1302.6244","created_at":"2026-05-18T03:19:13.136791+00:00"},{"alias_kind":"arxiv_version","alias_value":"1302.6244v2","created_at":"2026-05-18T03:19:13.136791+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1302.6244","created_at":"2026-05-18T03:19:13.136791+00:00"},{"alias_kind":"pith_short_12","alias_value":"CI5WSAPJMHKX","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_16","alias_value":"CI5WSAPJMHKXLAHM","created_at":"2026-05-18T12:27:40.988391+00:00"},{"alias_kind":"pith_short_8","alias_value":"CI5WSAPJ","created_at":"2026-05-18T12:27:40.988391+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2607.01315","citing_title":"Discovery of an Inflated Hot Neptune and Its Formation from Jovian Mass Loss","ref_index":211,"is_internal_anchor":true},{"citing_arxiv_id":"2606.30799","citing_title":"The GAPS programme at TNG ?. TOI-1533: a compact system hosting a super-Neptune-mass pair with disparate radii","ref_index":99,"is_internal_anchor":true},{"citing_arxiv_id":"2606.30722","citing_title":"Chemical Abundances of the Bioessential Elements C, O and S, and the Refractory Elements Fe and Ni, in Solar-type Exoplanet-hosting Stars from HARPS North and South","ref_index":113,"is_internal_anchor":true},{"citing_arxiv_id":"2606.12010","citing_title":"The 35-Myr old infant planet TOI-837 b has a mildly misaligned orbit","ref_index":97,"is_internal_anchor":true},{"citing_arxiv_id":"2606.20224","citing_title":"TOI-2147 b and TOI-6019 b: Two eccentric warm Jupiters detected and characterized with TESS and MaHPS","ref_index":24,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW","json":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW.json","graph_json":"https://pith.science/api/pith-number/CI5WSAPJMHKXLAHMYPVFCE6PNW/graph.json","events_json":"https://pith.science/api/pith-number/CI5WSAPJMHKXLAHMYPVFCE6PNW/events.json","paper":"https://pith.science/paper/CI5WSAPJ"},"agent_actions":{"view_html":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW","download_json":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW.json","view_paper":"https://pith.science/paper/CI5WSAPJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1302.6244&json=true","fetch_graph":"https://pith.science/api/pith-number/CI5WSAPJMHKXLAHMYPVFCE6PNW/graph.json","fetch_events":"https://pith.science/api/pith-number/CI5WSAPJMHKXLAHMYPVFCE6PNW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW/action/storage_attestation","attest_author":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW/action/author_attestation","sign_citation":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW/action/citation_signature","submit_replication":"https://pith.science/pith/CI5WSAPJMHKXLAHMYPVFCE6PNW/action/replication_record"}},"created_at":"2026-05-18T03:19:13.136791+00:00","updated_at":"2026-05-18T03:19:13.136791+00:00"}