{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:OEODSRMPWAYAY5NTW4VM47W7KZ","short_pith_number":"pith:OEODSRMP","schema_version":"1.0","canonical_sha256":"711c39458fb0300c75b3b72ace7edf5647d8d75e781a93ab81eaa6b04489b30f","source":{"kind":"arxiv","id":"2405.05055","version":2},"attestation_state":"computed","paper":{"title":"Over 200 globular clusters in the Milky Way and still none with super-Solar metallicity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Minniti, E. R. Garro, J. G. Fern\\'andez-Trincado","submitted_at":"2024-05-08T13:48:21Z","abstract_excerpt":"Many globular clusters (GCs) in the Milky Way (MW) have been studied in recent years, especially in hidden regions such as those of the Galactic bulge. Our main goal is to understand what we can learn if we include these new objects into the MWGC system that we know today. We catalogue 37 recently discovered GCs. We use different distributions for investigating the MWGC system: metallicity distribution (MD), luminosity function (LF), and age distribution. We first treat separately the new GCs sample from the known and well-characterised GCs. We merge these two samples, upgrading the MWGC syste"},"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":"2405.05055","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-05-08T13:48:21Z","cross_cats_sorted":[],"title_canon_sha256":"23b9c14d31a17b913c2db5234d35ee3a413f568f3b782d66155e4d22c25bd592","abstract_canon_sha256":"b0d14f24cf9e61721a1f7759e8ce64abda63379b81f9c3ce7224c8d720358764"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:20:11.436072Z","signature_b64":"D23Gs373JWtu5I0v5W9aabL9uZ8YQ1Tq5X4y65jnAjqLuVASFcQpYWKQT3f2RyRkkUtnm5pwg7Qe/jz9DEGoAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"711c39458fb0300c75b3b72ace7edf5647d8d75e781a93ab81eaa6b04489b30f","last_reissued_at":"2026-07-05T08:20:11.435654Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:20:11.435654Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Over 200 globular clusters in the Milky Way and still none with super-Solar metallicity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"D. Minniti, E. R. Garro, J. G. Fern\\'andez-Trincado","submitted_at":"2024-05-08T13:48:21Z","abstract_excerpt":"Many globular clusters (GCs) in the Milky Way (MW) have been studied in recent years, especially in hidden regions such as those of the Galactic bulge. Our main goal is to understand what we can learn if we include these new objects into the MWGC system that we know today. We catalogue 37 recently discovered GCs. We use different distributions for investigating the MWGC system: metallicity distribution (MD), luminosity function (LF), and age distribution. We first treat separately the new GCs sample from the known and well-characterised GCs. We merge these two samples, upgrading the MWGC syste"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.05055","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2405.05055/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2405.05055","created_at":"2026-07-05T08:20:11.435715+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.05055v2","created_at":"2026-07-05T08:20:11.435715+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.05055","created_at":"2026-07-05T08:20:11.435715+00:00"},{"alias_kind":"pith_short_12","alias_value":"OEODSRMPWAYA","created_at":"2026-07-05T08:20:11.435715+00:00"},{"alias_kind":"pith_short_16","alias_value":"OEODSRMPWAYAY5NT","created_at":"2026-07-05T08:20:11.435715+00:00"},{"alias_kind":"pith_short_8","alias_value":"OEODSRMP","created_at":"2026-07-05T08:20:11.435715+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.13930","citing_title":"Bayesian Analysis of Gravitational Wave Microlensing Effects from Galactic Double White Dwarfs","ref_index":55,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ","json":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ.json","graph_json":"https://pith.science/api/pith-number/OEODSRMPWAYAY5NTW4VM47W7KZ/graph.json","events_json":"https://pith.science/api/pith-number/OEODSRMPWAYAY5NTW4VM47W7KZ/events.json","paper":"https://pith.science/paper/OEODSRMP"},"agent_actions":{"view_html":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ","download_json":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ.json","view_paper":"https://pith.science/paper/OEODSRMP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.05055&json=true","fetch_graph":"https://pith.science/api/pith-number/OEODSRMPWAYAY5NTW4VM47W7KZ/graph.json","fetch_events":"https://pith.science/api/pith-number/OEODSRMPWAYAY5NTW4VM47W7KZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ/action/storage_attestation","attest_author":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ/action/author_attestation","sign_citation":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ/action/citation_signature","submit_replication":"https://pith.science/pith/OEODSRMPWAYAY5NTW4VM47W7KZ/action/replication_record"}},"created_at":"2026-07-05T08:20:11.435715+00:00","updated_at":"2026-07-05T08:20:11.435715+00:00"}