{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:5HF5SHLOO4BPHWHCDRI2MKJAIU","short_pith_number":"pith:5HF5SHLO","schema_version":"1.0","canonical_sha256":"e9cbd91d6e7702f3d8e21c51a629204537a22d8f3ab7b72a7c1cc84636cf6ded","source":{"kind":"arxiv","id":"1309.2014","version":1},"attestation_state":"computed","paper":{"title":"Local Group and Star Cluster Dynamics from HSTPROMO (The Hubble Space Telescope Proper Motion Collaboration)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alis Deason, Andrea Bellini, Danny Lennon, Davide Massari, Eileen Meyer, Elena Sabbi, Gurtina Besla, Imants Platais, Jay Anderson, Julio Chaname, Laura Watkins, Mario Soto, Michele Trenti, Mike Boylan-Kolchin, Nitya Kallivayalil, Paolo Bianchini, Puragra Guhathakurta, Roeland P. van der Marel, Sangmo Tony Sohn, Tuan Do","submitted_at":"2013-09-08T22:15:10Z","abstract_excerpt":"The Hubble Space Telescope (HST) has proven to be uniquely suited for the measurement of proper motions (PMs) of stars and galaxies in the nearby Universe. Here we summarize the main results and ongoing studies of the HSTPROMO collaboration, which over the past decade has executed some two dozen observational and theoretical HST projects on this topic. This is continuing to revolutionize our dynamical understanding of many objects, including: globular clusters; young star clusters; stars and stellar streams in the Milky Way halo; Local Group galaxies, including dwarf satellite galaxies, the Ma"},"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":"1309.2014","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-09-08T22:15:10Z","cross_cats_sorted":[],"title_canon_sha256":"5c7d3cbf20633984489b9c0e3bf73dec8fbf0ab3038b17baa46ba69a64df50e0","abstract_canon_sha256":"08f0b22e200d2d3cd2e0ddc77479815bd889647cdc2cdcb56cd1053edc53d112"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:13:56.761307Z","signature_b64":"NNF93+9xBL+bMHbEQ1udVfQeSPSNW3BKJ8gg3dnVvh9eeyGWZKTo07uVCTEC9bjh3lg2WsnZlcIz31q9DEIbCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e9cbd91d6e7702f3d8e21c51a629204537a22d8f3ab7b72a7c1cc84636cf6ded","last_reissued_at":"2026-05-18T03:13:56.760627Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:13:56.760627Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Local Group and Star Cluster Dynamics from HSTPROMO (The Hubble Space Telescope Proper Motion Collaboration)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alis Deason, Andrea Bellini, Danny Lennon, Davide Massari, Eileen Meyer, Elena Sabbi, Gurtina Besla, Imants Platais, Jay Anderson, Julio Chaname, Laura Watkins, Mario Soto, Michele Trenti, Mike Boylan-Kolchin, Nitya Kallivayalil, Paolo Bianchini, Puragra Guhathakurta, Roeland P. van der Marel, Sangmo Tony Sohn, Tuan Do","submitted_at":"2013-09-08T22:15:10Z","abstract_excerpt":"The Hubble Space Telescope (HST) has proven to be uniquely suited for the measurement of proper motions (PMs) of stars and galaxies in the nearby Universe. Here we summarize the main results and ongoing studies of the HSTPROMO collaboration, which over the past decade has executed some two dozen observational and theoretical HST projects on this topic. This is continuing to revolutionize our dynamical understanding of many objects, including: globular clusters; young star clusters; stars and stellar streams in the Milky Way halo; Local Group galaxies, including dwarf satellite galaxies, the Ma"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1309.2014","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":"1309.2014","created_at":"2026-05-18T03:13:56.760721+00:00"},{"alias_kind":"arxiv_version","alias_value":"1309.2014v1","created_at":"2026-05-18T03:13:56.760721+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1309.2014","created_at":"2026-05-18T03:13:56.760721+00:00"},{"alias_kind":"pith_short_12","alias_value":"5HF5SHLOO4BP","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"5HF5SHLOO4BPHWHC","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"5HF5SHLO","created_at":"2026-05-18T12:27:34.582898+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/5HF5SHLOO4BPHWHCDRI2MKJAIU","json":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU.json","graph_json":"https://pith.science/api/pith-number/5HF5SHLOO4BPHWHCDRI2MKJAIU/graph.json","events_json":"https://pith.science/api/pith-number/5HF5SHLOO4BPHWHCDRI2MKJAIU/events.json","paper":"https://pith.science/paper/5HF5SHLO"},"agent_actions":{"view_html":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU","download_json":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU.json","view_paper":"https://pith.science/paper/5HF5SHLO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1309.2014&json=true","fetch_graph":"https://pith.science/api/pith-number/5HF5SHLOO4BPHWHCDRI2MKJAIU/graph.json","fetch_events":"https://pith.science/api/pith-number/5HF5SHLOO4BPHWHCDRI2MKJAIU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU/action/storage_attestation","attest_author":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU/action/author_attestation","sign_citation":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU/action/citation_signature","submit_replication":"https://pith.science/pith/5HF5SHLOO4BPHWHCDRI2MKJAIU/action/replication_record"}},"created_at":"2026-05-18T03:13:56.760721+00:00","updated_at":"2026-05-18T03:13:56.760721+00:00"}