{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:PM32GWUCIUUJQDHEIZLCSKNR2Q","short_pith_number":"pith:PM32GWUC","schema_version":"1.0","canonical_sha256":"7b37a35a824528980ce446562929b1d4160b80447c87bcc60f6a3d8bfcf86afb","source":{"kind":"arxiv","id":"1312.2272","version":2},"attestation_state":"computed","paper":{"title":"On the kinematic separation of field and cluster stars across the Bulge globular NGC 6528","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Aparicio, A. Calamida, A.P. Milone, A.Walker, E. P. Lagioia, G. Bono, G. Iannicola, I. Ferraro, M. Dall'Ora, M. Monelli, N. Matsunaga, P. B. Stetson, P. G. Prada Moroni, R. Buonanno, R. Gilmozzi","submitted_at":"2013-12-08T22:11:26Z","abstract_excerpt":"We present deep and precise multi-band photometry of the Galactic Bulge globular cluster NGC6528. The current dataset includes optical and near-infrared images collected with ACS/WFC, WFC3/UVIS, and WFC3/IR on board the Hubble Space Telescope. The images cover a time interval of almost ten years and we have been able to carry out a proper-motion separation between cluster and field stars. We performed a detailed comparison in the m_F814W, m_F606W - m_F814W Color-Magnitude Diagram with two empirical calibrators observed in the same bands. We found that NGC6528 is coeval with and more metal-rich"},"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":"1312.2272","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-12-08T22:11:26Z","cross_cats_sorted":[],"title_canon_sha256":"5cd999e691bbf0160ec6e8840322a386cc862e53815073d957eabecc5d2f31f7","abstract_canon_sha256":"193cb50e559054f7a7d34f678371cdbb66fd972b971d223bde30089d6e793570"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:57:06.320703Z","signature_b64":"NB74UfF7yUBY9KFOSm8rEux5k8/y6db4JVCB0E/UrP747JBkOB4+Ge491g36XJUaog2T7b1ubPKRaKqTM9RXDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7b37a35a824528980ce446562929b1d4160b80447c87bcc60f6a3d8bfcf86afb","last_reissued_at":"2026-05-18T02:57:06.320071Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:57:06.320071Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the kinematic separation of field and cluster stars across the Bulge globular NGC 6528","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Aparicio, A. Calamida, A.P. Milone, A.Walker, E. P. Lagioia, G. Bono, G. Iannicola, I. Ferraro, M. Dall'Ora, M. Monelli, N. Matsunaga, P. B. Stetson, P. G. Prada Moroni, R. Buonanno, R. Gilmozzi","submitted_at":"2013-12-08T22:11:26Z","abstract_excerpt":"We present deep and precise multi-band photometry of the Galactic Bulge globular cluster NGC6528. The current dataset includes optical and near-infrared images collected with ACS/WFC, WFC3/UVIS, and WFC3/IR on board the Hubble Space Telescope. The images cover a time interval of almost ten years and we have been able to carry out a proper-motion separation between cluster and field stars. We performed a detailed comparison in the m_F814W, m_F606W - m_F814W Color-Magnitude Diagram with two empirical calibrators observed in the same bands. We found that NGC6528 is coeval with and more metal-rich"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.2272","kind":"arxiv","version":2},"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":"1312.2272","created_at":"2026-05-18T02:57:06.320158+00:00"},{"alias_kind":"arxiv_version","alias_value":"1312.2272v2","created_at":"2026-05-18T02:57:06.320158+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.2272","created_at":"2026-05-18T02:57:06.320158+00:00"},{"alias_kind":"pith_short_12","alias_value":"PM32GWUCIUUJ","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_16","alias_value":"PM32GWUCIUUJQDHE","created_at":"2026-05-18T12:27:54.935989+00:00"},{"alias_kind":"pith_short_8","alias_value":"PM32GWUC","created_at":"2026-05-18T12:27:54.935989+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.20979","citing_title":"Globular Clusters in the Time of the JWST. I. Survey Design and First Results on Multiple Populations and Beyond","ref_index":72,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q","json":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q.json","graph_json":"https://pith.science/api/pith-number/PM32GWUCIUUJQDHEIZLCSKNR2Q/graph.json","events_json":"https://pith.science/api/pith-number/PM32GWUCIUUJQDHEIZLCSKNR2Q/events.json","paper":"https://pith.science/paper/PM32GWUC"},"agent_actions":{"view_html":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q","download_json":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q.json","view_paper":"https://pith.science/paper/PM32GWUC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1312.2272&json=true","fetch_graph":"https://pith.science/api/pith-number/PM32GWUCIUUJQDHEIZLCSKNR2Q/graph.json","fetch_events":"https://pith.science/api/pith-number/PM32GWUCIUUJQDHEIZLCSKNR2Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q/action/storage_attestation","attest_author":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q/action/author_attestation","sign_citation":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q/action/citation_signature","submit_replication":"https://pith.science/pith/PM32GWUCIUUJQDHEIZLCSKNR2Q/action/replication_record"}},"created_at":"2026-05-18T02:57:06.320158+00:00","updated_at":"2026-05-18T02:57:06.320158+00:00"}