{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:2DHUYDMF4REMVBPFYKAXTGZ42A","short_pith_number":"pith:2DHUYDMF","schema_version":"1.0","canonical_sha256":"d0cf4c0d85e448ca85e5c281799b3cd03b5f2bbcd9d946a674b84eb2c8cd6e46","source":{"kind":"arxiv","id":"2502.01748","version":1},"attestation_state":"computed","paper":{"title":"Resolving the Super-Earth/Gas Giant Connection in Stellar Mass and Metallicity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Eve J. Lee, Marta L. Bryan","submitted_at":"2025-02-03T19:00:10Z","abstract_excerpt":"The observed correlation between inner super-Earths and outer gas giants places strong constraints on formation theories. Building on previous work, Bryan $\\&$ Lee 2024 showed that there is a statistically significant positive correlation between super-Earths and outer gas giants around metal-rich FGK stars, and that this correlation disappears for metal-poor hosts. Here we consider how this connection evolves across stellar mass. Starting with our sample of 85 M-dwarfs ($<$0.6 M$_{\\odot}$) hosting inner super-Earths, we calculate P(GG|SE, [Fe/H]$>$0) = 9.4 (+10.2 -3.1)$\\%$ and P(GG|SE, [Fe/H]"},"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":"2502.01748","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.EP","submitted_at":"2025-02-03T19:00:10Z","cross_cats_sorted":["astro-ph.GA","astro-ph.SR"],"title_canon_sha256":"c0c1439a402477b2a15e83b1fdf9e5b8f6a443c32ac64101492eedd3ae40b0e0","abstract_canon_sha256":"a064dc1788ea2c62adb62ba2ba2d0c13f40b24e90869ca529b49f97b6bfc768c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:09:18.567111Z","signature_b64":"ossAu9pvsZ5KcZdocs6f4pqN9Qeo3X9SC90V+prLQc5T8bp7HGz8UAFHMm9Gb5z553KfKrKo+4cAKVSX0JoJBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d0cf4c0d85e448ca85e5c281799b3cd03b5f2bbcd9d946a674b84eb2c8cd6e46","last_reissued_at":"2026-07-05T10:09:18.566674Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:09:18.566674Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resolving the Super-Earth/Gas Giant Connection in Stellar Mass and Metallicity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"Eve J. Lee, Marta L. Bryan","submitted_at":"2025-02-03T19:00:10Z","abstract_excerpt":"The observed correlation between inner super-Earths and outer gas giants places strong constraints on formation theories. Building on previous work, Bryan $\\&$ Lee 2024 showed that there is a statistically significant positive correlation between super-Earths and outer gas giants around metal-rich FGK stars, and that this correlation disappears for metal-poor hosts. Here we consider how this connection evolves across stellar mass. Starting with our sample of 85 M-dwarfs ($<$0.6 M$_{\\odot}$) hosting inner super-Earths, we calculate P(GG|SE, [Fe/H]$>$0) = 9.4 (+10.2 -3.1)$\\%$ and P(GG|SE, [Fe/H]"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.01748","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/2502.01748/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":"2502.01748","created_at":"2026-07-05T10:09:18.566737+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.01748v1","created_at":"2026-07-05T10:09:18.566737+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.01748","created_at":"2026-07-05T10:09:18.566737+00:00"},{"alias_kind":"pith_short_12","alias_value":"2DHUYDMF4REM","created_at":"2026-07-05T10:09:18.566737+00:00"},{"alias_kind":"pith_short_16","alias_value":"2DHUYDMF4REMVBPF","created_at":"2026-07-05T10:09:18.566737+00:00"},{"alias_kind":"pith_short_8","alias_value":"2DHUYDMF","created_at":"2026-07-05T10:09:18.566737+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.12524","citing_title":"An early look at how gas giants shape small planet bulk compositions","ref_index":8,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A","json":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A.json","graph_json":"https://pith.science/api/pith-number/2DHUYDMF4REMVBPFYKAXTGZ42A/graph.json","events_json":"https://pith.science/api/pith-number/2DHUYDMF4REMVBPFYKAXTGZ42A/events.json","paper":"https://pith.science/paper/2DHUYDMF"},"agent_actions":{"view_html":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A","download_json":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A.json","view_paper":"https://pith.science/paper/2DHUYDMF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.01748&json=true","fetch_graph":"https://pith.science/api/pith-number/2DHUYDMF4REMVBPFYKAXTGZ42A/graph.json","fetch_events":"https://pith.science/api/pith-number/2DHUYDMF4REMVBPFYKAXTGZ42A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A/action/storage_attestation","attest_author":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A/action/author_attestation","sign_citation":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A/action/citation_signature","submit_replication":"https://pith.science/pith/2DHUYDMF4REMVBPFYKAXTGZ42A/action/replication_record"}},"created_at":"2026-07-05T10:09:18.566737+00:00","updated_at":"2026-07-05T10:09:18.566737+00:00"}