{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:I6VKLMQHL22NRORNR66EIPZT52","short_pith_number":"pith:I6VKLMQH","schema_version":"1.0","canonical_sha256":"47aaa5b2075eb4d8ba2d8fbc443f33ee963ce41080da0c99084fe5c370362854","source":{"kind":"arxiv","id":"1903.10513","version":1},"attestation_state":"computed","paper":{"title":"Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Benoit Famaey, James S. Bullock, Marcel S. Pawlowski, Tyler Kelley","submitted_at":"2019-03-25T18:00:02Z","abstract_excerpt":"The Milky Way, the Andromeda galaxy, and Centaurus A host flattened distributions of satellite galaxies which exhibits coherent velocity trends indicative of rotation. Comparably extreme satellite structures are very rare in cosmological LCDM simulations, giving rise to the `satellite plane problem'. As a possible explanation it has been suggested that earlier-forming, higher concentration host halos contain more flattened and kinematically coherent satellite planes. We have tested for such a proposed correlation between the satellite plane and host halo properties in the ELVIS suite of simula"},"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":"1903.10513","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-03-25T18:00:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"1fb46535e1bbea49e57d2591d35b339ab6192940be379bba9de329a49e65bd80","abstract_canon_sha256":"3efdb6080bd0e1b47eb6b7e99b1e5f3cc4f728a300e8ee1702d5344bf5ab546a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:47:16.624701Z","signature_b64":"M/FjmJlaJjVMj1AH0HJC298/qEZjFXwgA2h6RLRMeALlsHB5PipESadyOccOnjMyH8IGDqvEVoCKT8fsAUL5DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"47aaa5b2075eb4d8ba2d8fbc443f33ee963ce41080da0c99084fe5c370362854","last_reissued_at":"2026-05-17T23:47:16.624333Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:47:16.624333Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Benoit Famaey, James S. Bullock, Marcel S. Pawlowski, Tyler Kelley","submitted_at":"2019-03-25T18:00:02Z","abstract_excerpt":"The Milky Way, the Andromeda galaxy, and Centaurus A host flattened distributions of satellite galaxies which exhibits coherent velocity trends indicative of rotation. Comparably extreme satellite structures are very rare in cosmological LCDM simulations, giving rise to the `satellite plane problem'. As a possible explanation it has been suggested that earlier-forming, higher concentration host halos contain more flattened and kinematically coherent satellite planes. We have tested for such a proposed correlation between the satellite plane and host halo properties in the ELVIS suite of simula"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.10513","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":""},"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":"1903.10513","created_at":"2026-05-17T23:47:16.624395+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.10513v1","created_at":"2026-05-17T23:47:16.624395+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.10513","created_at":"2026-05-17T23:47:16.624395+00:00"},{"alias_kind":"pith_short_12","alias_value":"I6VKLMQHL22N","created_at":"2026-05-18T12:33:18.533446+00:00"},{"alias_kind":"pith_short_16","alias_value":"I6VKLMQHL22NRORN","created_at":"2026-05-18T12:33:18.533446+00:00"},{"alias_kind":"pith_short_8","alias_value":"I6VKLMQH","created_at":"2026-05-18T12:33:18.533446+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/I6VKLMQHL22NRORNR66EIPZT52","json":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52.json","graph_json":"https://pith.science/api/pith-number/I6VKLMQHL22NRORNR66EIPZT52/graph.json","events_json":"https://pith.science/api/pith-number/I6VKLMQHL22NRORNR66EIPZT52/events.json","paper":"https://pith.science/paper/I6VKLMQH"},"agent_actions":{"view_html":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52","download_json":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52.json","view_paper":"https://pith.science/paper/I6VKLMQH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.10513&json=true","fetch_graph":"https://pith.science/api/pith-number/I6VKLMQHL22NRORNR66EIPZT52/graph.json","fetch_events":"https://pith.science/api/pith-number/I6VKLMQHL22NRORNR66EIPZT52/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52/action/storage_attestation","attest_author":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52/action/author_attestation","sign_citation":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52/action/citation_signature","submit_replication":"https://pith.science/pith/I6VKLMQHL22NRORNR66EIPZT52/action/replication_record"}},"created_at":"2026-05-17T23:47:16.624395+00:00","updated_at":"2026-05-17T23:47:16.624395+00:00"}