{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:UDPVDD2X5RZWX4BTWUFG5WOS5K","short_pith_number":"pith:UDPVDD2X","schema_version":"1.0","canonical_sha256":"a0df518f57ec736bf033b50a6ed9d2ea8ca30c618ab172566240df31037bd417","source":{"kind":"arxiv","id":"1506.00957","version":1},"attestation_state":"computed","paper":{"title":"Star Streams in Triaxial Isochrone Potentials with Sub-Halos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Raymond G. Carlberg","submitted_at":"2015-06-02T16:49:53Z","abstract_excerpt":"The velocity, position, and action variable evolution of a tidal stream drawn out of a star cluster in a triaxial isochrone potential containing a sub-halo population reproduces many of the orbital effects of more general cosmological halos but allows easy calculation of orbital actions. We employ a spherical shell code which we show accurately reproduces the results of a tree gravity code for a collisionless star cluster. Streams from clusters on high eccentricity orbits, $e\\gtrsim 0.6$, can spread out so much that the amount of material at high enough surface density to stand out on the sky "},"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":"1506.00957","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2015-06-02T16:49:53Z","cross_cats_sorted":[],"title_canon_sha256":"cab8821956f5bbb560c3a4b243ef56ddb225998fb1cb89ae405e98376d9f46fb","abstract_canon_sha256":"45d34053b62f39b625cd4d8d83744a9dbe0760f2f445177fe9200386e02cf72d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:47.391483Z","signature_b64":"02qujjhcfTOa3URVjl+b08IoGdBnRnm5kTjRniTPs2nnNPx21NafmVFBi/G77lEnRP/YyR4F7FD6t/7krT0uDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a0df518f57ec736bf033b50a6ed9d2ea8ca30c618ab172566240df31037bd417","last_reissued_at":"2026-05-18T01:35:47.390817Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:47.390817Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Star Streams in Triaxial Isochrone Potentials with Sub-Halos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Raymond G. Carlberg","submitted_at":"2015-06-02T16:49:53Z","abstract_excerpt":"The velocity, position, and action variable evolution of a tidal stream drawn out of a star cluster in a triaxial isochrone potential containing a sub-halo population reproduces many of the orbital effects of more general cosmological halos but allows easy calculation of orbital actions. We employ a spherical shell code which we show accurately reproduces the results of a tree gravity code for a collisionless star cluster. Streams from clusters on high eccentricity orbits, $e\\gtrsim 0.6$, can spread out so much that the amount of material at high enough surface density to stand out on the sky "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.00957","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":"1506.00957","created_at":"2026-05-18T01:35:47.390941+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.00957v1","created_at":"2026-05-18T01:35:47.390941+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.00957","created_at":"2026-05-18T01:35:47.390941+00:00"},{"alias_kind":"pith_short_12","alias_value":"UDPVDD2X5RZW","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_16","alias_value":"UDPVDD2X5RZWX4BT","created_at":"2026-05-18T12:29:44.643036+00:00"},{"alias_kind":"pith_short_8","alias_value":"UDPVDD2X","created_at":"2026-05-18T12:29:44.643036+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/UDPVDD2X5RZWX4BTWUFG5WOS5K","json":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K.json","graph_json":"https://pith.science/api/pith-number/UDPVDD2X5RZWX4BTWUFG5WOS5K/graph.json","events_json":"https://pith.science/api/pith-number/UDPVDD2X5RZWX4BTWUFG5WOS5K/events.json","paper":"https://pith.science/paper/UDPVDD2X"},"agent_actions":{"view_html":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K","download_json":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K.json","view_paper":"https://pith.science/paper/UDPVDD2X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.00957&json=true","fetch_graph":"https://pith.science/api/pith-number/UDPVDD2X5RZWX4BTWUFG5WOS5K/graph.json","fetch_events":"https://pith.science/api/pith-number/UDPVDD2X5RZWX4BTWUFG5WOS5K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K/action/storage_attestation","attest_author":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K/action/author_attestation","sign_citation":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K/action/citation_signature","submit_replication":"https://pith.science/pith/UDPVDD2X5RZWX4BTWUFG5WOS5K/action/replication_record"}},"created_at":"2026-05-18T01:35:47.390941+00:00","updated_at":"2026-05-18T01:35:47.390941+00:00"}