{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QZ64MDPTGFQKRC26MCLF4AROIH","short_pith_number":"pith:QZ64MDPT","schema_version":"1.0","canonical_sha256":"867dc60df33160a88b5e60965e022e41f20d3fcf77171851dfad57deb01affa7","source":{"kind":"arxiv","id":"1611.03753","version":1},"attestation_state":"computed","paper":{"title":"Properties of Star Clusters -- III: Analysis of 13 FSR Clusters using UKIDSS-GPS and VISTA-VVV","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.S.M. Buckner, D. Froebrich","submitted_at":"2016-11-11T15:46:02Z","abstract_excerpt":"Discerning the nature of open cluster candidates is essential for both individual and statistical analyses of cluster properties. Here we establish the nature of thirteen cluster candidates from the FSR cluster list using photometry from the 2MASS and deeper, higher resolution UKIDSS-GPS and VISTA-VVV surveys. These clusters were selected because they were flagged in our previous studies as expected to contain a large proportion of pre-main sequence members or are at unusually small/large Galactocentric distances. We employ a decontamination procedure of JHK photometry to identify cluster memb"},"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":"1611.03753","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-11T15:46:02Z","cross_cats_sorted":[],"title_canon_sha256":"3628cfe72dbee02c1406d3685e2af4eee34a52ac6822083fc224a55c92a9ed74","abstract_canon_sha256":"260237410bd18f3edc6b6bbaeb0d4fe7ffdba4b37204aa18b06a6c6923a39552"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:59:33.435054Z","signature_b64":"grel/9/x3QM1hoImv6Mkv4snHEVfZ/9fGzs+A8tPUybI9imKFokp7Zz/zCcrtsHDj7hnT8DryxLJrmLBscB2AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"867dc60df33160a88b5e60965e022e41f20d3fcf77171851dfad57deb01affa7","last_reissued_at":"2026-05-18T00:59:33.434390Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:59:33.434390Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Properties of Star Clusters -- III: Analysis of 13 FSR Clusters using UKIDSS-GPS and VISTA-VVV","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A.S.M. Buckner, D. Froebrich","submitted_at":"2016-11-11T15:46:02Z","abstract_excerpt":"Discerning the nature of open cluster candidates is essential for both individual and statistical analyses of cluster properties. Here we establish the nature of thirteen cluster candidates from the FSR cluster list using photometry from the 2MASS and deeper, higher resolution UKIDSS-GPS and VISTA-VVV surveys. These clusters were selected because they were flagged in our previous studies as expected to contain a large proportion of pre-main sequence members or are at unusually small/large Galactocentric distances. We employ a decontamination procedure of JHK photometry to identify cluster memb"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.03753","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":"1611.03753","created_at":"2026-05-18T00:59:33.434501+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.03753v1","created_at":"2026-05-18T00:59:33.434501+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.03753","created_at":"2026-05-18T00:59:33.434501+00:00"},{"alias_kind":"pith_short_12","alias_value":"QZ64MDPTGFQK","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_16","alias_value":"QZ64MDPTGFQKRC26","created_at":"2026-05-18T12:30:41.710351+00:00"},{"alias_kind":"pith_short_8","alias_value":"QZ64MDPT","created_at":"2026-05-18T12:30:41.710351+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/QZ64MDPTGFQKRC26MCLF4AROIH","json":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH.json","graph_json":"https://pith.science/api/pith-number/QZ64MDPTGFQKRC26MCLF4AROIH/graph.json","events_json":"https://pith.science/api/pith-number/QZ64MDPTGFQKRC26MCLF4AROIH/events.json","paper":"https://pith.science/paper/QZ64MDPT"},"agent_actions":{"view_html":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH","download_json":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH.json","view_paper":"https://pith.science/paper/QZ64MDPT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.03753&json=true","fetch_graph":"https://pith.science/api/pith-number/QZ64MDPTGFQKRC26MCLF4AROIH/graph.json","fetch_events":"https://pith.science/api/pith-number/QZ64MDPTGFQKRC26MCLF4AROIH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH/action/storage_attestation","attest_author":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH/action/author_attestation","sign_citation":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH/action/citation_signature","submit_replication":"https://pith.science/pith/QZ64MDPTGFQKRC26MCLF4AROIH/action/replication_record"}},"created_at":"2026-05-18T00:59:33.434501+00:00","updated_at":"2026-05-18T00:59:33.434501+00:00"}