{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:NSCFJYAD253JWUJ5VY2YOD4LAS","short_pith_number":"pith:NSCFJYAD","schema_version":"1.0","canonical_sha256":"6c8454e003d7769b513dae35870f8b048b4b08c4fc59002c80162cb72992005c","source":{"kind":"arxiv","id":"1904.04261","version":1},"attestation_state":"computed","paper":{"title":"The E-MOSAICS project: tracing galaxy formation and assembly with the age-metallicity distribution of globular clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. M. Diederik Kruijssen (Heidelberg), Joel L. Pfeffer (LJMU), Nate Bastian (LJMU), Robert A. Crain (LJMU)","submitted_at":"2019-04-08T18:00:03Z","abstract_excerpt":"We present 25 cosmological zoom-in simulations of Milky Way-mass galaxies in the `MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE' (E-MOSAICS) project. E-MOSAICS couples a detailed physical model for the formation, evolution, and disruption of star clusters to the EAGLE galaxy formation simulations. This enables following the co-formation and co-evolution of galaxies and their star cluster populations, thus realising the long-standing promise of using globular clusters (GCs) as tracers of galaxy formation and assembly. The simulations show that the age-metal"},"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":"1904.04261","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-04-08T18:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"77bc4f74d250c59179171bf2998764d0e05426e3aa58065c52455fb3ec6245af","abstract_canon_sha256":"e9e0bc3fc0e5a60eaa68b989c5f0809b38b640addeb4e9570235e4aede69df7d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:48:29.430506Z","signature_b64":"dfHsMxuFngZWsXYg1Qhr1r+VjkAq3rVxg1mHGOe9IINzUoG2AkRbyq2yStGuaXqIE4YmmBytAAyOIVaUt3e5Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6c8454e003d7769b513dae35870f8b048b4b08c4fc59002c80162cb72992005c","last_reissued_at":"2026-05-17T23:48:29.429935Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:48:29.429935Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The E-MOSAICS project: tracing galaxy formation and assembly with the age-metallicity distribution of globular clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. M. Diederik Kruijssen (Heidelberg), Joel L. Pfeffer (LJMU), Nate Bastian (LJMU), Robert A. Crain (LJMU)","submitted_at":"2019-04-08T18:00:03Z","abstract_excerpt":"We present 25 cosmological zoom-in simulations of Milky Way-mass galaxies in the `MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE' (E-MOSAICS) project. E-MOSAICS couples a detailed physical model for the formation, evolution, and disruption of star clusters to the EAGLE galaxy formation simulations. This enables following the co-formation and co-evolution of galaxies and their star cluster populations, thus realising the long-standing promise of using globular clusters (GCs) as tracers of galaxy formation and assembly. The simulations show that the age-metal"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.04261","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":"1904.04261","created_at":"2026-05-17T23:48:29.430039+00:00"},{"alias_kind":"arxiv_version","alias_value":"1904.04261v1","created_at":"2026-05-17T23:48:29.430039+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1904.04261","created_at":"2026-05-17T23:48:29.430039+00:00"},{"alias_kind":"pith_short_12","alias_value":"NSCFJYAD253J","created_at":"2026-05-18T12:33:24.271573+00:00"},{"alias_kind":"pith_short_16","alias_value":"NSCFJYAD253JWUJ5","created_at":"2026-05-18T12:33:24.271573+00:00"},{"alias_kind":"pith_short_8","alias_value":"NSCFJYAD","created_at":"2026-05-18T12:33:24.271573+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2603.07481","citing_title":"New Way to Date Globular Clusters: Brown Dwarf Cooling Sequences","ref_index":142,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS","json":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS.json","graph_json":"https://pith.science/api/pith-number/NSCFJYAD253JWUJ5VY2YOD4LAS/graph.json","events_json":"https://pith.science/api/pith-number/NSCFJYAD253JWUJ5VY2YOD4LAS/events.json","paper":"https://pith.science/paper/NSCFJYAD"},"agent_actions":{"view_html":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS","download_json":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS.json","view_paper":"https://pith.science/paper/NSCFJYAD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1904.04261&json=true","fetch_graph":"https://pith.science/api/pith-number/NSCFJYAD253JWUJ5VY2YOD4LAS/graph.json","fetch_events":"https://pith.science/api/pith-number/NSCFJYAD253JWUJ5VY2YOD4LAS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS/action/storage_attestation","attest_author":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS/action/author_attestation","sign_citation":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS/action/citation_signature","submit_replication":"https://pith.science/pith/NSCFJYAD253JWUJ5VY2YOD4LAS/action/replication_record"}},"created_at":"2026-05-17T23:48:29.430039+00:00","updated_at":"2026-05-17T23:48:29.430039+00:00"}