{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:5243PFQPFMAFDL4P6ST7S746P5","short_pith_number":"pith:5243PFQP","schema_version":"1.0","canonical_sha256":"eeb9b7960f2b0051af8ff4a7f97f9e7f4e1cb719a1683d8d2cd0f0c5e136015a","source":{"kind":"arxiv","id":"2007.14473","version":2},"attestation_state":"computed","paper":{"title":"Architectures of Exoplanetary Systems. III: Eccentricity and Mutual Inclination Distributions of AMD-stable Planetary Systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Daniel Carrera, Darin Ragozzine, Eric B. Ford, Matthias Y. He","submitted_at":"2020-07-28T20:30:27Z","abstract_excerpt":"The angular momentum deficit (AMD) of a planetary system is a measure of its orbital excitation and a predictor of long-term stability. We adopt the AMD-stability criteria to constrain the orbital architectures for exoplanetary systems. Previously, He, Ford, & Ragozzine (2019) (arXiv:1907.07773v2) showed through forward modelling (SysSim) that the observed multiplicity distribution can be well reproduced by two populations consisting of a low and a high mutual inclination component. Here, we show that a broad distribution of mutual inclinations arising from systems at the AMD-stability limit c"},"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":"2007.14473","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2020-07-28T20:30:27Z","cross_cats_sorted":[],"title_canon_sha256":"dbab95265dfa69a31d5bc66916651050efd59c74f45a6ff7060dc4aa76adfdf2","abstract_canon_sha256":"2fbf23744d8606c846433ce415cc1749fbc01053e67c6c2e6f55c35ffc2b9484"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:58:11.100088Z","signature_b64":"A/l1OHtzpqtnmdv0Ybc+6Dscqo0/wGRGo559497D6yth/Bf+sLhZNvvZqwG1OxLHcIf9DhIiVLu7icbu7FAGCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eeb9b7960f2b0051af8ff4a7f97f9e7f4e1cb719a1683d8d2cd0f0c5e136015a","last_reissued_at":"2026-07-05T01:58:11.099632Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:58:11.099632Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Architectures of Exoplanetary Systems. III: Eccentricity and Mutual Inclination Distributions of AMD-stable Planetary Systems","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"Daniel Carrera, Darin Ragozzine, Eric B. Ford, Matthias Y. He","submitted_at":"2020-07-28T20:30:27Z","abstract_excerpt":"The angular momentum deficit (AMD) of a planetary system is a measure of its orbital excitation and a predictor of long-term stability. We adopt the AMD-stability criteria to constrain the orbital architectures for exoplanetary systems. Previously, He, Ford, & Ragozzine (2019) (arXiv:1907.07773v2) showed through forward modelling (SysSim) that the observed multiplicity distribution can be well reproduced by two populations consisting of a low and a high mutual inclination component. Here, we show that a broad distribution of mutual inclinations arising from systems at the AMD-stability limit c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.14473","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/2007.14473/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":"2007.14473","created_at":"2026-07-05T01:58:11.099696+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.14473v2","created_at":"2026-07-05T01:58:11.099696+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.14473","created_at":"2026-07-05T01:58:11.099696+00:00"},{"alias_kind":"pith_short_12","alias_value":"5243PFQPFMAF","created_at":"2026-07-05T01:58:11.099696+00:00"},{"alias_kind":"pith_short_16","alias_value":"5243PFQPFMAFDL4P","created_at":"2026-07-05T01:58:11.099696+00:00"},{"alias_kind":"pith_short_8","alias_value":"5243PFQP","created_at":"2026-07-05T01:58:11.099696+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.09451","citing_title":"Companion Architectures of Sub-Saturns: Distinct Migration Pathways Across the Neptunian Landscape","ref_index":151,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5","json":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5.json","graph_json":"https://pith.science/api/pith-number/5243PFQPFMAFDL4P6ST7S746P5/graph.json","events_json":"https://pith.science/api/pith-number/5243PFQPFMAFDL4P6ST7S746P5/events.json","paper":"https://pith.science/paper/5243PFQP"},"agent_actions":{"view_html":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5","download_json":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5.json","view_paper":"https://pith.science/paper/5243PFQP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.14473&json=true","fetch_graph":"https://pith.science/api/pith-number/5243PFQPFMAFDL4P6ST7S746P5/graph.json","fetch_events":"https://pith.science/api/pith-number/5243PFQPFMAFDL4P6ST7S746P5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5/action/storage_attestation","attest_author":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5/action/author_attestation","sign_citation":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5/action/citation_signature","submit_replication":"https://pith.science/pith/5243PFQPFMAFDL4P6ST7S746P5/action/replication_record"}},"created_at":"2026-07-05T01:58:11.099696+00:00","updated_at":"2026-07-05T01:58:11.099696+00:00"}