{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:7Z7R3TNVCNEGAO4RIJ5Q3SVFIE","short_pith_number":"pith:7Z7R3TNV","canonical_record":{"source":{"id":"1712.00019","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-30T19:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"1a52857e53fc74a34ad477cd82c8900d93de4c41ee98ebc6da3b85649a7fcdd7","abstract_canon_sha256":"2c5498008133e87df6fdfa7d130cc442f6029075cf74a324396a9eed1c515d2a"},"schema_version":"1.0"},"canonical_sha256":"fe7f1dcdb51348603b91427b0dcaa54135ebd98ed595d3ac22b837da2746f8fd","source":{"kind":"arxiv","id":"1712.00019","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1712.00019","created_at":"2026-05-18T00:22:27Z"},{"alias_kind":"arxiv_version","alias_value":"1712.00019v1","created_at":"2026-05-18T00:22:27Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.00019","created_at":"2026-05-18T00:22:27Z"},{"alias_kind":"pith_short_12","alias_value":"7Z7R3TNVCNEG","created_at":"2026-05-18T12:31:05Z"},{"alias_kind":"pith_short_16","alias_value":"7Z7R3TNVCNEGAO4R","created_at":"2026-05-18T12:31:05Z"},{"alias_kind":"pith_short_8","alias_value":"7Z7R3TNV","created_at":"2026-05-18T12:31:05Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:7Z7R3TNVCNEGAO4RIJ5Q3SVFIE","target":"record","payload":{"canonical_record":{"source":{"id":"1712.00019","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-30T19:00:03Z","cross_cats_sorted":[],"title_canon_sha256":"1a52857e53fc74a34ad477cd82c8900d93de4c41ee98ebc6da3b85649a7fcdd7","abstract_canon_sha256":"2c5498008133e87df6fdfa7d130cc442f6029075cf74a324396a9eed1c515d2a"},"schema_version":"1.0"},"canonical_sha256":"fe7f1dcdb51348603b91427b0dcaa54135ebd98ed595d3ac22b837da2746f8fd","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:27.036142Z","signature_b64":"VEeGilRbjhZM1QdOFsPIHnBBLOxIflscQWoCWiMdBSwrOMVnbrq1Hrx3+r4J+fImN3ToMKhH0oJvxKE0BmXCAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fe7f1dcdb51348603b91427b0dcaa54135ebd98ed595d3ac22b837da2746f8fd","last_reissued_at":"2026-05-18T00:22:27.035466Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:27.035466Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1712.00019","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:22:27Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"QFK22GGsp2nMoH2/ipS+Lkc1bwmQg8fwGD5HfmsVjXx5wB/ReXxA/sDQ7Klzczy29m/pNF0VJqfeFsi1/yBTCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-02T23:04:54.175207Z"},"content_sha256":"829dd3f43da542c605cdedc31174137e4a2cf2bb9e2542c9b9a5219fa902135c","schema_version":"1.0","event_id":"sha256:829dd3f43da542c605cdedc31174137e4a2cf2bb9e2542c9b9a5219fa902135c"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:7Z7R3TNVCNEGAO4RIJ5Q3SVFIE","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The E-MOSAICS Project: simulating the formation and co-evolution of galaxies and their star cluster populations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. M. Diederik Kruijssen, Joel Pfeffer, Nate Bastian, Robert A. Crain","submitted_at":"2017-11-30T19:00:03Z","abstract_excerpt":"We introduce the MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models describing the formation, evolution and disruption of star clusters into the EAGLE galaxy formation simulations, enabling the examination of the co-evolution of star clusters and their host galaxies in a fully cosmological context. A fraction of the star formation rate of dense gas is assumed to yield a cluster population; this fraction, and the population's initial properties, are governed by the physical properties of the natal gas. The subse"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.00019","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:22:27Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"UjYi7RAQX74F/n1RsgZ9N2AwCxO28Nl7WRoQKzCwvB7YkvdK4szkuVHatZiDe5T0E9hSppLeFUew28lWRmlNBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-02T23:04:54.175568Z"},"content_sha256":"1f1bbd3028f4f96d4cfeee473749772705a8677d5d9a0d2f24b0e68434b26efe","schema_version":"1.0","event_id":"sha256:1f1bbd3028f4f96d4cfeee473749772705a8677d5d9a0d2f24b0e68434b26efe"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/7Z7R3TNVCNEGAO4RIJ5Q3SVFIE/bundle.json","state_url":"https://pith.science/pith/7Z7R3TNVCNEGAO4RIJ5Q3SVFIE/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/7Z7R3TNVCNEGAO4RIJ5Q3SVFIE/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-07-02T23:04:54Z","links":{"resolver":"https://pith.science/pith/7Z7R3TNVCNEGAO4RIJ5Q3SVFIE","bundle":"https://pith.science/pith/7Z7R3TNVCNEGAO4RIJ5Q3SVFIE/bundle.json","state":"https://pith.science/pith/7Z7R3TNVCNEGAO4RIJ5Q3SVFIE/state.json","well_known_bundle":"https://pith.science/.well-known/pith/7Z7R3TNVCNEGAO4RIJ5Q3SVFIE/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:7Z7R3TNVCNEGAO4RIJ5Q3SVFIE","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"2c5498008133e87df6fdfa7d130cc442f6029075cf74a324396a9eed1c515d2a","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-30T19:00:03Z","title_canon_sha256":"1a52857e53fc74a34ad477cd82c8900d93de4c41ee98ebc6da3b85649a7fcdd7"},"schema_version":"1.0","source":{"id":"1712.00019","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1712.00019","created_at":"2026-05-18T00:22:27Z"},{"alias_kind":"arxiv_version","alias_value":"1712.00019v1","created_at":"2026-05-18T00:22:27Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.00019","created_at":"2026-05-18T00:22:27Z"},{"alias_kind":"pith_short_12","alias_value":"7Z7R3TNVCNEG","created_at":"2026-05-18T12:31:05Z"},{"alias_kind":"pith_short_16","alias_value":"7Z7R3TNVCNEGAO4R","created_at":"2026-05-18T12:31:05Z"},{"alias_kind":"pith_short_8","alias_value":"7Z7R3TNV","created_at":"2026-05-18T12:31:05Z"}],"graph_snapshots":[{"event_id":"sha256:1f1bbd3028f4f96d4cfeee473749772705a8677d5d9a0d2f24b0e68434b26efe","target":"graph","created_at":"2026-05-18T00:22:27Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We introduce the MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models describing the formation, evolution and disruption of star clusters into the EAGLE galaxy formation simulations, enabling the examination of the co-evolution of star clusters and their host galaxies in a fully cosmological context. A fraction of the star formation rate of dense gas is assumed to yield a cluster population; this fraction, and the population's initial properties, are governed by the physical properties of the natal gas. The subse","authors_text":"J. M. Diederik Kruijssen, Joel Pfeffer, Nate Bastian, Robert A. Crain","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-30T19:00:03Z","title":"The E-MOSAICS Project: simulating the formation and co-evolution of galaxies and their star cluster populations"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.00019","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:829dd3f43da542c605cdedc31174137e4a2cf2bb9e2542c9b9a5219fa902135c","target":"record","created_at":"2026-05-18T00:22:27Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"2c5498008133e87df6fdfa7d130cc442f6029075cf74a324396a9eed1c515d2a","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-11-30T19:00:03Z","title_canon_sha256":"1a52857e53fc74a34ad477cd82c8900d93de4c41ee98ebc6da3b85649a7fcdd7"},"schema_version":"1.0","source":{"id":"1712.00019","kind":"arxiv","version":1}},"canonical_sha256":"fe7f1dcdb51348603b91427b0dcaa54135ebd98ed595d3ac22b837da2746f8fd","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"fe7f1dcdb51348603b91427b0dcaa54135ebd98ed595d3ac22b837da2746f8fd","first_computed_at":"2026-05-18T00:22:27.035466Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:22:27.035466Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"VEeGilRbjhZM1QdOFsPIHnBBLOxIflscQWoCWiMdBSwrOMVnbrq1Hrx3+r4J+fImN3ToMKhH0oJvxKE0BmXCAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T00:22:27.036142Z","signed_message":"canonical_sha256_bytes"},"source_id":"1712.00019","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:829dd3f43da542c605cdedc31174137e4a2cf2bb9e2542c9b9a5219fa902135c","sha256:1f1bbd3028f4f96d4cfeee473749772705a8677d5d9a0d2f24b0e68434b26efe"],"state_sha256":"141f53e6a1887f1842641e2e0558eefd047af3ac68af66b29fec756c7377167e"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"MePwr9zlCJkI+c68hhhXK3gTye7qoLQz1v4ODItMNFEmAG5YW5uf1aqH6O7e9HPCLlgTdVk+rbbl/NYiGgYtCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-02T23:04:54.177550Z","bundle_sha256":"e30081ba7354010f5e4329d1942fc883bff9666c2bdeaeb004ff96c0883beb69"}}