{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:LMOHDHZI4ZFEGPQJKLU4CFTAIP","short_pith_number":"pith:LMOHDHZI","schema_version":"1.0","canonical_sha256":"5b1c719f28e64a433e0952e9c1166043d859fd7ad47b9de9b60032c85e7598ca","source":{"kind":"arxiv","id":"1406.1183","version":1},"attestation_state":"computed","paper":{"title":"Stellar-Encounter Driven Red-Giant Star Mass-Loss in Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. De Luca, A. Moraghan, C. Chung, E. Brocato, G. Raimondo, M. Pasquato, R. Carini, Y.-W. Lee","submitted_at":"2014-06-04T20:00:22Z","abstract_excerpt":"Globular Cluster (GC) Color-Magnitude Diagrams (CMDs) are reasonably well understood in terms of standard stellar-evolution. However, there are still some open issues, such as fully accounting for the Horizontal Branch (HB) morphology in terms of chemical and dynamical parameters. Mass-loss on the Red Giant Branch (RGB) shapes the mass-distribution of the HB stars, and the color distribution in turn. The physical mechanisms driving mass-loss are still unclear, as direct observations fail to reveal a clear correlation between mass-loss rate and stellar properties. The horizontal-branch mass-dis"},"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":"1406.1183","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2014-06-04T20:00:22Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"12515568c6db50f7b8271963921601018b80b01ece30c71f47088fb507543de7","abstract_canon_sha256":"e716a89829916867dd2be3a6fe1dd1abd80f9bdb48172982fb468458d92f9d50"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:02.061441Z","signature_b64":"8I3P+xyzLdZJq4AJtvDAjI7m5EHzdmVopsvDLsTQ4wDx2qEWJPYfsb20O9zS/yLCTSKR+Pf356qTCOIwKcwvCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b1c719f28e64a433e0952e9c1166043d859fd7ad47b9de9b60032c85e7598ca","last_reissued_at":"2026-05-18T01:43:02.061085Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:02.061085Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Stellar-Encounter Driven Red-Giant Star Mass-Loss in Globular Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.SR","authors_text":"A. De Luca, A. Moraghan, C. Chung, E. Brocato, G. Raimondo, M. Pasquato, R. Carini, Y.-W. Lee","submitted_at":"2014-06-04T20:00:22Z","abstract_excerpt":"Globular Cluster (GC) Color-Magnitude Diagrams (CMDs) are reasonably well understood in terms of standard stellar-evolution. However, there are still some open issues, such as fully accounting for the Horizontal Branch (HB) morphology in terms of chemical and dynamical parameters. Mass-loss on the Red Giant Branch (RGB) shapes the mass-distribution of the HB stars, and the color distribution in turn. The physical mechanisms driving mass-loss are still unclear, as direct observations fail to reveal a clear correlation between mass-loss rate and stellar properties. The horizontal-branch mass-dis"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1406.1183","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":"1406.1183","created_at":"2026-05-18T01:43:02.061140+00:00"},{"alias_kind":"arxiv_version","alias_value":"1406.1183v1","created_at":"2026-05-18T01:43:02.061140+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1406.1183","created_at":"2026-05-18T01:43:02.061140+00:00"},{"alias_kind":"pith_short_12","alias_value":"LMOHDHZI4ZFE","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_16","alias_value":"LMOHDHZI4ZFEGPQJ","created_at":"2026-05-18T12:28:38.356838+00:00"},{"alias_kind":"pith_short_8","alias_value":"LMOHDHZI","created_at":"2026-05-18T12:28:38.356838+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/LMOHDHZI4ZFEGPQJKLU4CFTAIP","json":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP.json","graph_json":"https://pith.science/api/pith-number/LMOHDHZI4ZFEGPQJKLU4CFTAIP/graph.json","events_json":"https://pith.science/api/pith-number/LMOHDHZI4ZFEGPQJKLU4CFTAIP/events.json","paper":"https://pith.science/paper/LMOHDHZI"},"agent_actions":{"view_html":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP","download_json":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP.json","view_paper":"https://pith.science/paper/LMOHDHZI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1406.1183&json=true","fetch_graph":"https://pith.science/api/pith-number/LMOHDHZI4ZFEGPQJKLU4CFTAIP/graph.json","fetch_events":"https://pith.science/api/pith-number/LMOHDHZI4ZFEGPQJKLU4CFTAIP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP/action/storage_attestation","attest_author":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP/action/author_attestation","sign_citation":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP/action/citation_signature","submit_replication":"https://pith.science/pith/LMOHDHZI4ZFEGPQJKLU4CFTAIP/action/replication_record"}},"created_at":"2026-05-18T01:43:02.061140+00:00","updated_at":"2026-05-18T01:43:02.061140+00:00"}