{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:2PUOAWHCF6A4EY2T5SXCOLHDJN","short_pith_number":"pith:2PUOAWHC","schema_version":"1.0","canonical_sha256":"d3e8e058e22f81c26353ecae272ce34b49c4a589dbd499786f3daeac244cee1f","source":{"kind":"arxiv","id":"2308.12340","version":1},"attestation_state":"computed","paper":{"title":"The progenitors of the intra-cluster light and intra-cluster globular clusters in galaxy groups and clusters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrew Benson, Jessica E. Doppel, Laura V. Sales, Niusha Ahvazi, Richard D'Souza, Vicente Rodriguez-Gomez","submitted_at":"2023-08-23T18:00:02Z","abstract_excerpt":"We use the IllustrisTNG50 cosmological hydrodynamical simulation, complemented by a catalog of tagged globular clusters, to investigate the properties and build up of two extended luminous components: the intra-cluster light (ICL) and the intra-cluster globular clusters (ICGC). We select the 39 most massive groups and clusters in the box, spanning the range of virial masses $5 \\times 10^{12} < \\rm M_{200}/\\rm M_{\\odot} < 2 \\times 10^{14}$. We find good agreement between predictions from the simulations and current observational estimates of the fraction of mass in the ICL and its radial extens"},"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":"2308.12340","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-08-23T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"c5b12ecd0f400950cf0c8ac3ec7d997db574b88162ba6f06b6ff66bac8bb0989","abstract_canon_sha256":"7b5d020464554b2d636fac51b8cb3af3300b9816693e9823c4e2f3398a56e250"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:44:10.551507Z","signature_b64":"wF8WE2jHsEIO7qkCFZqNBdmZvSVMIG382IRwPAQEWVSuNypWz9CQTovmtjoq+WawW/VoXcXapzg8XU1IOAyqDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d3e8e058e22f81c26353ecae272ce34b49c4a589dbd499786f3daeac244cee1f","last_reissued_at":"2026-07-05T06:44:10.551071Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:44:10.551071Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The progenitors of the intra-cluster light and intra-cluster globular clusters in galaxy groups and clusters","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrew Benson, Jessica E. Doppel, Laura V. Sales, Niusha Ahvazi, Richard D'Souza, Vicente Rodriguez-Gomez","submitted_at":"2023-08-23T18:00:02Z","abstract_excerpt":"We use the IllustrisTNG50 cosmological hydrodynamical simulation, complemented by a catalog of tagged globular clusters, to investigate the properties and build up of two extended luminous components: the intra-cluster light (ICL) and the intra-cluster globular clusters (ICGC). We select the 39 most massive groups and clusters in the box, spanning the range of virial masses $5 \\times 10^{12} < \\rm M_{200}/\\rm M_{\\odot} < 2 \\times 10^{14}$. We find good agreement between predictions from the simulations and current observational estimates of the fraction of mass in the ICL and its radial extens"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.12340","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2308.12340/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":"2308.12340","created_at":"2026-07-05T06:44:10.551136+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.12340v1","created_at":"2026-07-05T06:44:10.551136+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.12340","created_at":"2026-07-05T06:44:10.551136+00:00"},{"alias_kind":"pith_short_12","alias_value":"2PUOAWHCF6A4","created_at":"2026-07-05T06:44:10.551136+00:00"},{"alias_kind":"pith_short_16","alias_value":"2PUOAWHCF6A4EY2T","created_at":"2026-07-05T06:44:10.551136+00:00"},{"alias_kind":"pith_short_8","alias_value":"2PUOAWHC","created_at":"2026-07-05T06:44:10.551136+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.05158","citing_title":"Relationship between 2D and 3D Galaxy Stellar Mass and Correlations with Halo Mass","ref_index":66,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN","json":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN.json","graph_json":"https://pith.science/api/pith-number/2PUOAWHCF6A4EY2T5SXCOLHDJN/graph.json","events_json":"https://pith.science/api/pith-number/2PUOAWHCF6A4EY2T5SXCOLHDJN/events.json","paper":"https://pith.science/paper/2PUOAWHC"},"agent_actions":{"view_html":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN","download_json":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN.json","view_paper":"https://pith.science/paper/2PUOAWHC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.12340&json=true","fetch_graph":"https://pith.science/api/pith-number/2PUOAWHCF6A4EY2T5SXCOLHDJN/graph.json","fetch_events":"https://pith.science/api/pith-number/2PUOAWHCF6A4EY2T5SXCOLHDJN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN/action/storage_attestation","attest_author":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN/action/author_attestation","sign_citation":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN/action/citation_signature","submit_replication":"https://pith.science/pith/2PUOAWHCF6A4EY2T5SXCOLHDJN/action/replication_record"}},"created_at":"2026-07-05T06:44:10.551136+00:00","updated_at":"2026-07-05T06:44:10.551136+00:00"}