{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:YL2SQOJQ5AWCH2EA3BYAPECUVI","short_pith_number":"pith:YL2SQOJQ","schema_version":"1.0","canonical_sha256":"c2f5283930e82c23e880d870079054aa32909af41b03cb30d6f2cf9448de19f2","source":{"kind":"arxiv","id":"1706.09074","version":1},"attestation_state":"computed","paper":{"title":"The Peculiar Globular Cluster Palomar 1 and Persistence in the SDSS-APOGEE Database","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Charli M. Sakari, Collin L. Kielty, Farbod Jahandar, Jo Bovy, Kim A. Venn, Matthew D. Shetrone, Mike Irwin, Peter M. Frinchaboy, Ruth A. R. Digby","submitted_at":"2017-06-27T23:36:01Z","abstract_excerpt":"The SDSS-III APOGEE DR12 is a unique resource to search for stars beyond the tidal radii of star clusters. We have examined the APOGEE DR12 database for new candidates of the young star cluster Palomar 1, a system with previously reported tidal tails (Niederste-Ostholt et al. 2010). The APOGEE ASPCAP database includes spectra and stellar parameters for two known members of Pal 1 (Stars I and II), however these do not agree with the stellar parameters determined from optical spectra by Sakari et al. (2011). We find that the APOGEE analysis of these two stars is strongly affected by the known pe"},"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":"1706.09074","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-06-27T23:36:01Z","cross_cats_sorted":[],"title_canon_sha256":"f0e39ccdbba62de95b482a6bb621b3e8a7e66a14b5cb54dcc20d298ab0c62a1e","abstract_canon_sha256":"8fc5002ff26684a5ba154b7b4e0a9421df8fbf2262f6c706b3f2f7b48b6c588c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:41:19.976183Z","signature_b64":"loe3XdZm8syt/Hj2NCKpCD5Cq3LBMfbNg+1P/7jzsa3RyHTn9jEJWVYArnTy3Phgy2fdNhQnZvbo2G29LAdDDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c2f5283930e82c23e880d870079054aa32909af41b03cb30d6f2cf9448de19f2","last_reissued_at":"2026-05-18T00:41:19.975660Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:41:19.975660Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Peculiar Globular Cluster Palomar 1 and Persistence in the SDSS-APOGEE Database","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Charli M. Sakari, Collin L. Kielty, Farbod Jahandar, Jo Bovy, Kim A. Venn, Matthew D. Shetrone, Mike Irwin, Peter M. Frinchaboy, Ruth A. R. Digby","submitted_at":"2017-06-27T23:36:01Z","abstract_excerpt":"The SDSS-III APOGEE DR12 is a unique resource to search for stars beyond the tidal radii of star clusters. We have examined the APOGEE DR12 database for new candidates of the young star cluster Palomar 1, a system with previously reported tidal tails (Niederste-Ostholt et al. 2010). The APOGEE ASPCAP database includes spectra and stellar parameters for two known members of Pal 1 (Stars I and II), however these do not agree with the stellar parameters determined from optical spectra by Sakari et al. (2011). We find that the APOGEE analysis of these two stars is strongly affected by the known pe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.09074","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":"1706.09074","created_at":"2026-05-18T00:41:19.975742+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.09074v1","created_at":"2026-05-18T00:41:19.975742+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.09074","created_at":"2026-05-18T00:41:19.975742+00:00"},{"alias_kind":"pith_short_12","alias_value":"YL2SQOJQ5AWC","created_at":"2026-05-18T12:31:56.362134+00:00"},{"alias_kind":"pith_short_16","alias_value":"YL2SQOJQ5AWCH2EA","created_at":"2026-05-18T12:31:56.362134+00:00"},{"alias_kind":"pith_short_8","alias_value":"YL2SQOJQ","created_at":"2026-05-18T12:31:56.362134+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/YL2SQOJQ5AWCH2EA3BYAPECUVI","json":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI.json","graph_json":"https://pith.science/api/pith-number/YL2SQOJQ5AWCH2EA3BYAPECUVI/graph.json","events_json":"https://pith.science/api/pith-number/YL2SQOJQ5AWCH2EA3BYAPECUVI/events.json","paper":"https://pith.science/paper/YL2SQOJQ"},"agent_actions":{"view_html":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI","download_json":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI.json","view_paper":"https://pith.science/paper/YL2SQOJQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.09074&json=true","fetch_graph":"https://pith.science/api/pith-number/YL2SQOJQ5AWCH2EA3BYAPECUVI/graph.json","fetch_events":"https://pith.science/api/pith-number/YL2SQOJQ5AWCH2EA3BYAPECUVI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI/action/storage_attestation","attest_author":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI/action/author_attestation","sign_citation":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI/action/citation_signature","submit_replication":"https://pith.science/pith/YL2SQOJQ5AWCH2EA3BYAPECUVI/action/replication_record"}},"created_at":"2026-05-18T00:41:19.975742+00:00","updated_at":"2026-05-18T00:41:19.975742+00:00"}