{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:4EIBDXWVSGMWOJQLNDYLJJUD3J","short_pith_number":"pith:4EIBDXWV","schema_version":"1.0","canonical_sha256":"e11011ded5919967260b68f0b4a683da66b6ec36712cb7be7a5d36bf574de129","source":{"kind":"arxiv","id":"1905.09908","version":3},"attestation_state":"computed","paper":{"title":"Three-Component Kinematics of Multiple Stellar Populations in Globular Clusters with Gaia and VLT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A.F. Marino, A. Mastrobuono-Battisti, A.P. Milone, E.P. Lagioia, G. Cordoni, H. Baumgardt, M. Hilker, M. Tailo","submitted_at":"2019-05-23T20:29:03Z","abstract_excerpt":"The internal dynamics of multiple stellar populations in Globular Clusters (GCs) provides unique constraints on the physical processes responsible for their formation. Specifically, the present-day kinematics of cluster stars, such as rotation and velocity-dispersion, could be related to the initial configuration of the system. In recent work, we provided the first study of the kinematics of different stellar populations in NGC$\\,$0104 over a large field of view in the plane of the sky, exploiting Gaia Data Release 2 (DR2) proper motions combined with multi-band ground-based photometry. In thi"},"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":"1905.09908","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2019-05-23T20:29:03Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"19c83efc827965ed5326f2f016b624155b6ddc56312f8524847f78a1663b305b","abstract_canon_sha256":"c8dc78f37ef25b906486dfa28d653bc92adb13d1bb0e91b42056433a255998fa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:38:02.059677Z","signature_b64":"BRXUjI27k2U6zEIP/tf+aSc+addxIkll2Rx0UUcf4Ia/yPvicXdK7avyIcn4N2gaZWHPq/VpzJv3rZGdAgWvBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e11011ded5919967260b68f0b4a683da66b6ec36712cb7be7a5d36bf574de129","last_reissued_at":"2026-07-05T00:38:02.059251Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:38:02.059251Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Three-Component Kinematics of Multiple Stellar Populations in Globular Clusters with Gaia and VLT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A.F. Marino, A. Mastrobuono-Battisti, A.P. Milone, E.P. Lagioia, G. Cordoni, H. Baumgardt, M. Hilker, M. Tailo","submitted_at":"2019-05-23T20:29:03Z","abstract_excerpt":"The internal dynamics of multiple stellar populations in Globular Clusters (GCs) provides unique constraints on the physical processes responsible for their formation. Specifically, the present-day kinematics of cluster stars, such as rotation and velocity-dispersion, could be related to the initial configuration of the system. In recent work, we provided the first study of the kinematics of different stellar populations in NGC$\\,$0104 over a large field of view in the plane of the sky, exploiting Gaia Data Release 2 (DR2) proper motions combined with multi-band ground-based photometry. In thi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.09908","kind":"arxiv","version":3},"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/1905.09908/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":"1905.09908","created_at":"2026-07-05T00:38:02.059305+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.09908v3","created_at":"2026-07-05T00:38:02.059305+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.09908","created_at":"2026-07-05T00:38:02.059305+00:00"},{"alias_kind":"pith_short_12","alias_value":"4EIBDXWVSGMW","created_at":"2026-07-05T00:38:02.059305+00:00"},{"alias_kind":"pith_short_16","alias_value":"4EIBDXWVSGMWOJQL","created_at":"2026-07-05T00:38:02.059305+00:00"},{"alias_kind":"pith_short_8","alias_value":"4EIBDXWV","created_at":"2026-07-05T00:38:02.059305+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/4EIBDXWVSGMWOJQLNDYLJJUD3J","json":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J.json","graph_json":"https://pith.science/api/pith-number/4EIBDXWVSGMWOJQLNDYLJJUD3J/graph.json","events_json":"https://pith.science/api/pith-number/4EIBDXWVSGMWOJQLNDYLJJUD3J/events.json","paper":"https://pith.science/paper/4EIBDXWV"},"agent_actions":{"view_html":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J","download_json":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J.json","view_paper":"https://pith.science/paper/4EIBDXWV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.09908&json=true","fetch_graph":"https://pith.science/api/pith-number/4EIBDXWVSGMWOJQLNDYLJJUD3J/graph.json","fetch_events":"https://pith.science/api/pith-number/4EIBDXWVSGMWOJQLNDYLJJUD3J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J/action/storage_attestation","attest_author":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J/action/author_attestation","sign_citation":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J/action/citation_signature","submit_replication":"https://pith.science/pith/4EIBDXWVSGMWOJQLNDYLJJUD3J/action/replication_record"}},"created_at":"2026-07-05T00:38:02.059305+00:00","updated_at":"2026-07-05T00:38:02.059305+00:00"}