{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:W7DWO3Q3PGBAAL6BL3WS2EVJON","short_pith_number":"pith:W7DWO3Q3","schema_version":"1.0","canonical_sha256":"b7c7676e1b7982002fc15eed2d12a97355aa4a8b8665594124944d8abdebc335","source":{"kind":"arxiv","id":"1801.04629","version":1},"attestation_state":"computed","paper":{"title":"Shape of LOSVD\\lowercase{s} in barred disks: Implications for future IFU surveys","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Juntai Shen, Martin Bureau, Min Du, Victor P. Debattista, Yingying Zhou, Zhao-Yu Li","submitted_at":"2018-01-15T00:49:36Z","abstract_excerpt":"The shape of LOSVDs (line-of-sight velocity distributions) carries important information about the internal dynamics of galaxies. The skewness of LOSVDs represents their asymmetric deviation from a Gaussian profile. Correlations between the skewness parameter ($h_3$) and the mean velocity (\\vm) of a Gauss-Hermite series reflect the underlying stellar orbital configurations of different morphological components. Using two self-consistent $N$-body simulations of disk galaxies with different bar strengths, we investigate \\hv\\ correlations at different inclination angles. Similar to previous studi"},"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":"1801.04629","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-01-15T00:49:36Z","cross_cats_sorted":[],"title_canon_sha256":"9e4cf45326efae2f51df512b641dd21ae3497caa3b2a33fbf14627c0d203124e","abstract_canon_sha256":"7da0d50d8bbcae1e4f88b7c32e487f6d1ef90ededcbc39ac0dfdbf01333dbd85"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:48:02.113970Z","signature_b64":"PXvBSAMVO9v6tPU186lO3cobIxjrwYvi3CXn7Izs0mrOsu0s0JhUqG91agg9OxYGo4sZaPNgoJkMI77/7zbmCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b7c7676e1b7982002fc15eed2d12a97355aa4a8b8665594124944d8abdebc335","last_reissued_at":"2026-05-17T23:48:02.113459Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:48:02.113459Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Shape of LOSVD\\lowercase{s} in barred disks: Implications for future IFU surveys","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Juntai Shen, Martin Bureau, Min Du, Victor P. Debattista, Yingying Zhou, Zhao-Yu Li","submitted_at":"2018-01-15T00:49:36Z","abstract_excerpt":"The shape of LOSVDs (line-of-sight velocity distributions) carries important information about the internal dynamics of galaxies. The skewness of LOSVDs represents their asymmetric deviation from a Gaussian profile. Correlations between the skewness parameter ($h_3$) and the mean velocity (\\vm) of a Gauss-Hermite series reflect the underlying stellar orbital configurations of different morphological components. Using two self-consistent $N$-body simulations of disk galaxies with different bar strengths, we investigate \\hv\\ correlations at different inclination angles. Similar to previous studi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.04629","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":"1801.04629","created_at":"2026-05-17T23:48:02.113544+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.04629v1","created_at":"2026-05-17T23:48:02.113544+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.04629","created_at":"2026-05-17T23:48:02.113544+00:00"},{"alias_kind":"pith_short_12","alias_value":"W7DWO3Q3PGBA","created_at":"2026-05-18T12:32:59.047623+00:00"},{"alias_kind":"pith_short_16","alias_value":"W7DWO3Q3PGBAAL6B","created_at":"2026-05-18T12:32:59.047623+00:00"},{"alias_kind":"pith_short_8","alias_value":"W7DWO3Q3","created_at":"2026-05-18T12:32:59.047623+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/W7DWO3Q3PGBAAL6BL3WS2EVJON","json":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON.json","graph_json":"https://pith.science/api/pith-number/W7DWO3Q3PGBAAL6BL3WS2EVJON/graph.json","events_json":"https://pith.science/api/pith-number/W7DWO3Q3PGBAAL6BL3WS2EVJON/events.json","paper":"https://pith.science/paper/W7DWO3Q3"},"agent_actions":{"view_html":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON","download_json":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON.json","view_paper":"https://pith.science/paper/W7DWO3Q3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.04629&json=true","fetch_graph":"https://pith.science/api/pith-number/W7DWO3Q3PGBAAL6BL3WS2EVJON/graph.json","fetch_events":"https://pith.science/api/pith-number/W7DWO3Q3PGBAAL6BL3WS2EVJON/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON/action/storage_attestation","attest_author":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON/action/author_attestation","sign_citation":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON/action/citation_signature","submit_replication":"https://pith.science/pith/W7DWO3Q3PGBAAL6BL3WS2EVJON/action/replication_record"}},"created_at":"2026-05-17T23:48:02.113544+00:00","updated_at":"2026-05-17T23:48:02.113544+00:00"}