{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:JAQ33M5ZT36CWOJ6IU4DXN3XYX","short_pith_number":"pith:JAQ33M5Z","schema_version":"1.0","canonical_sha256":"4821bdb3b99efc2b393e45383bb777c5e733765b3d3053b83e094fa05b83e8bd","source":{"kind":"arxiv","id":"1305.3645","version":1},"attestation_state":"computed","paper":{"title":"The Origin and Chemical Evolution of the Exotic Globular Cluster NGC3201","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"C. Mu\\~noz, D. Geisler, S. Villanova","submitted_at":"2013-05-15T21:34:34Z","abstract_excerpt":"NGC3201 is a globular cluster (GC) which shows very peculiar kinematic characteristics including an extreme radial velocity and a highly retrograde orbit, strongly suggesting an extraGalactic origin. Our aims are to study NGC3201 in the context of multiple populations (MPs), hoping to constrain possible candidates for the self-enrichment by studying the chemical abundance pattern, as well as adding insight into the origin of this intriguing cluster. We present a detailed chemical abundance analysis of eight red giant branch (RGB) stars using high resolution spectroscopy. We measured 29 element"},"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":"1305.3645","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2013-05-15T21:34:34Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"0d200b9a46c75ff813e1daf32c27e3b8b66009e9cd7313457f006eb690b42368","abstract_canon_sha256":"70133efa9be8cb43413bb3b23131ca015e7c3911676120c3610a740d44fecd1b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:56.678282Z","signature_b64":"O+CqXyFZzjQYayA+aYEhbGsZUdl78WNXmDjXo43JlyY4BNxL4SxIcRAxdh0yHlrWyYeUvmWPDfwuUj1uTPZ0Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4821bdb3b99efc2b393e45383bb777c5e733765b3d3053b83e094fa05b83e8bd","last_reissued_at":"2026-05-18T01:49:56.677855Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:56.677855Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Origin and Chemical Evolution of the Exotic Globular Cluster NGC3201","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"C. Mu\\~noz, D. Geisler, S. Villanova","submitted_at":"2013-05-15T21:34:34Z","abstract_excerpt":"NGC3201 is a globular cluster (GC) which shows very peculiar kinematic characteristics including an extreme radial velocity and a highly retrograde orbit, strongly suggesting an extraGalactic origin. Our aims are to study NGC3201 in the context of multiple populations (MPs), hoping to constrain possible candidates for the self-enrichment by studying the chemical abundance pattern, as well as adding insight into the origin of this intriguing cluster. We present a detailed chemical abundance analysis of eight red giant branch (RGB) stars using high resolution spectroscopy. We measured 29 element"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.3645","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":"1305.3645","created_at":"2026-05-18T01:49:56.677914+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.3645v1","created_at":"2026-05-18T01:49:56.677914+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.3645","created_at":"2026-05-18T01:49:56.677914+00:00"},{"alias_kind":"pith_short_12","alias_value":"JAQ33M5ZT36C","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_16","alias_value":"JAQ33M5ZT36CWOJ6","created_at":"2026-05-18T12:27:49.015174+00:00"},{"alias_kind":"pith_short_8","alias_value":"JAQ33M5Z","created_at":"2026-05-18T12:27:49.015174+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/JAQ33M5ZT36CWOJ6IU4DXN3XYX","json":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX.json","graph_json":"https://pith.science/api/pith-number/JAQ33M5ZT36CWOJ6IU4DXN3XYX/graph.json","events_json":"https://pith.science/api/pith-number/JAQ33M5ZT36CWOJ6IU4DXN3XYX/events.json","paper":"https://pith.science/paper/JAQ33M5Z"},"agent_actions":{"view_html":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX","download_json":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX.json","view_paper":"https://pith.science/paper/JAQ33M5Z","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.3645&json=true","fetch_graph":"https://pith.science/api/pith-number/JAQ33M5ZT36CWOJ6IU4DXN3XYX/graph.json","fetch_events":"https://pith.science/api/pith-number/JAQ33M5ZT36CWOJ6IU4DXN3XYX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX/action/storage_attestation","attest_author":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX/action/author_attestation","sign_citation":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX/action/citation_signature","submit_replication":"https://pith.science/pith/JAQ33M5ZT36CWOJ6IU4DXN3XYX/action/replication_record"}},"created_at":"2026-05-18T01:49:56.677914+00:00","updated_at":"2026-05-18T01:49:56.677914+00:00"}