{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:UR3BUKAJUL6GDOM5PVJ3WNVFQS","short_pith_number":"pith:UR3BUKAJ","schema_version":"1.0","canonical_sha256":"a4761a2809a2fc61b99d7d53bb36a584b909dfcc8f58179472e578478628592d","source":{"kind":"arxiv","id":"1911.12367","version":2},"attestation_state":"computed","paper":{"title":"The baryon content of groups and clusters of galaxies in the FABLE simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Debora Sijacki, Ewald Puchwein, Nicholas A. Henden","submitted_at":"2019-11-27T19:00:01Z","abstract_excerpt":"We study the gas and stellar mass content of galaxy groups and clusters in the FABLE suite of cosmological hydrodynamical simulations, including the evolution of their central brightest cluster galaxies (BCGs), satellite galaxies and intracluster light (ICL). The total gas and stellar mass of FABLE clusters are in very good agreement with observations and show negligible redshift evolution at fixed halo mass for $M_{500} \\gtrsim 3 \\times 10^{14} M_{\\odot}$ at $z \\lesssim 1$, in line with recent findings from Sunyaev-Zel'dovich (SZ)-selected cluster samples. Importantly, the simulations predict"},"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":"1911.12367","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2019-11-27T19:00:01Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"3ee4b21d847c7836dc7710708005dfded2ebba1b8e1364ef621d9d7fe752605d","abstract_canon_sha256":"32c0a01d0f1455c3618f715704647fe8408518d934ba0c0ed602cab87fb423fb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:38:56.415736Z","signature_b64":"8atWJMpUZFdj1T4L6oepGYofnSRsQYHJe1jiSfUQ3uKOA0Gti+1MjzhKjXOql0u1l4v7UtXbF8fdNqxE5FMTBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a4761a2809a2fc61b99d7d53bb36a584b909dfcc8f58179472e578478628592d","last_reissued_at":"2026-07-05T01:38:56.415393Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:38:56.415393Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The baryon content of groups and clusters of galaxies in the FABLE simulations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Debora Sijacki, Ewald Puchwein, Nicholas A. Henden","submitted_at":"2019-11-27T19:00:01Z","abstract_excerpt":"We study the gas and stellar mass content of galaxy groups and clusters in the FABLE suite of cosmological hydrodynamical simulations, including the evolution of their central brightest cluster galaxies (BCGs), satellite galaxies and intracluster light (ICL). The total gas and stellar mass of FABLE clusters are in very good agreement with observations and show negligible redshift evolution at fixed halo mass for $M_{500} \\gtrsim 3 \\times 10^{14} M_{\\odot}$ at $z \\lesssim 1$, in line with recent findings from Sunyaev-Zel'dovich (SZ)-selected cluster samples. Importantly, the simulations predict"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1911.12367","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/1911.12367/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":"1911.12367","created_at":"2026-07-05T01:38:56.415448+00:00"},{"alias_kind":"arxiv_version","alias_value":"1911.12367v2","created_at":"2026-07-05T01:38:56.415448+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1911.12367","created_at":"2026-07-05T01:38:56.415448+00:00"},{"alias_kind":"pith_short_12","alias_value":"UR3BUKAJUL6G","created_at":"2026-07-05T01:38:56.415448+00:00"},{"alias_kind":"pith_short_16","alias_value":"UR3BUKAJUL6GDOM5","created_at":"2026-07-05T01:38:56.415448+00:00"},{"alias_kind":"pith_short_8","alias_value":"UR3BUKAJ","created_at":"2026-07-05T01:38:56.415448+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.05208","citing_title":"Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations","ref_index":15,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS","json":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS.json","graph_json":"https://pith.science/api/pith-number/UR3BUKAJUL6GDOM5PVJ3WNVFQS/graph.json","events_json":"https://pith.science/api/pith-number/UR3BUKAJUL6GDOM5PVJ3WNVFQS/events.json","paper":"https://pith.science/paper/UR3BUKAJ"},"agent_actions":{"view_html":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS","download_json":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS.json","view_paper":"https://pith.science/paper/UR3BUKAJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1911.12367&json=true","fetch_graph":"https://pith.science/api/pith-number/UR3BUKAJUL6GDOM5PVJ3WNVFQS/graph.json","fetch_events":"https://pith.science/api/pith-number/UR3BUKAJUL6GDOM5PVJ3WNVFQS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS/action/storage_attestation","attest_author":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS/action/author_attestation","sign_citation":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS/action/citation_signature","submit_replication":"https://pith.science/pith/UR3BUKAJUL6GDOM5PVJ3WNVFQS/action/replication_record"}},"created_at":"2026-07-05T01:38:56.415448+00:00","updated_at":"2026-07-05T01:38:56.415448+00:00"}