{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:RNV6YALERJNX7GDB4X5RP3T73A","short_pith_number":"pith:RNV6YALE","schema_version":"1.0","canonical_sha256":"8b6bec01648a5b7f9861e5fb17ee7fd80a9019884bc7a66feb9f60d707064c93","source":{"kind":"arxiv","id":"1901.03832","version":1},"attestation_state":"computed","paper":{"title":"Study of Lithium Rich Giants with the GALAH Spectroscopic Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bacham Eswar Reddy, Deepak","submitted_at":"2019-01-12T09:34:22Z","abstract_excerpt":"In this article, we speculate on the possible mechanisms for Li enhancement origin in RGB stars based on a large data set of around 340,299 stars collected from the GALAH survey combined with the Gaia astrometry. Data has 51,982 low mass (M$\\leq$ 2M$_{\\odot}$) RGB stars with reliable atmospheric parameters. The data set shows a well populated RGB with well-defined luminosity bump and red clump with significant number of stars at each of these two key phases. We found 335 new Li-rich RGB stars with Li abundance, A(Li) $\\geq$ 1.80 $\\pm$ 0.14 dex, of which 20 are super Li-rich with A(Li) $\\geq$ 3"},"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":"1901.03832","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2019-01-12T09:34:22Z","cross_cats_sorted":[],"title_canon_sha256":"b801432527418c575ef2736e14394762e5f351789a6050a216aad0b3efe8fd5a","abstract_canon_sha256":"31d9c167232bcc2faab9b6fa2204cd7b7d8ca3db13bacf1b7e476324fd9dcae0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:55:26.869367Z","signature_b64":"dUMlGUL8iZaymOXvIybOqwBTmQA7M0PB6vOxQykGRK8jNeiVdvLBWe51YrBMRYPckTIs0Y3n7FBSe3zNcVlPBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8b6bec01648a5b7f9861e5fb17ee7fd80a9019884bc7a66feb9f60d707064c93","last_reissued_at":"2026-05-17T23:55:26.868990Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:55:26.868990Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Study of Lithium Rich Giants with the GALAH Spectroscopic Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Bacham Eswar Reddy, Deepak","submitted_at":"2019-01-12T09:34:22Z","abstract_excerpt":"In this article, we speculate on the possible mechanisms for Li enhancement origin in RGB stars based on a large data set of around 340,299 stars collected from the GALAH survey combined with the Gaia astrometry. Data has 51,982 low mass (M$\\leq$ 2M$_{\\odot}$) RGB stars with reliable atmospheric parameters. The data set shows a well populated RGB with well-defined luminosity bump and red clump with significant number of stars at each of these two key phases. We found 335 new Li-rich RGB stars with Li abundance, A(Li) $\\geq$ 1.80 $\\pm$ 0.14 dex, of which 20 are super Li-rich with A(Li) $\\geq$ 3"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1901.03832","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":"1901.03832","created_at":"2026-05-17T23:55:26.869044+00:00"},{"alias_kind":"arxiv_version","alias_value":"1901.03832v1","created_at":"2026-05-17T23:55:26.869044+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1901.03832","created_at":"2026-05-17T23:55:26.869044+00:00"},{"alias_kind":"pith_short_12","alias_value":"RNV6YALERJNX","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_16","alias_value":"RNV6YALERJNX7GDB","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_8","alias_value":"RNV6YALE","created_at":"2026-05-18T12:33:27.125529+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/RNV6YALERJNX7GDB4X5RP3T73A","json":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A.json","graph_json":"https://pith.science/api/pith-number/RNV6YALERJNX7GDB4X5RP3T73A/graph.json","events_json":"https://pith.science/api/pith-number/RNV6YALERJNX7GDB4X5RP3T73A/events.json","paper":"https://pith.science/paper/RNV6YALE"},"agent_actions":{"view_html":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A","download_json":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A.json","view_paper":"https://pith.science/paper/RNV6YALE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1901.03832&json=true","fetch_graph":"https://pith.science/api/pith-number/RNV6YALERJNX7GDB4X5RP3T73A/graph.json","fetch_events":"https://pith.science/api/pith-number/RNV6YALERJNX7GDB4X5RP3T73A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A/action/storage_attestation","attest_author":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A/action/author_attestation","sign_citation":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A/action/citation_signature","submit_replication":"https://pith.science/pith/RNV6YALERJNX7GDB4X5RP3T73A/action/replication_record"}},"created_at":"2026-05-17T23:55:26.869044+00:00","updated_at":"2026-05-17T23:55:26.869044+00:00"}