{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:3DB24XDXFJL7IYDD5NTUPX4JEL","short_pith_number":"pith:3DB24XDX","schema_version":"1.0","canonical_sha256":"d8c3ae5c772a57f46063eb6747df8922fc118452ced19450e57485f0d673a9a3","source":{"kind":"arxiv","id":"2009.06634","version":2},"attestation_state":"computed","paper":{"title":"Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Annalisa Pillepich, Nhut Truong, Norbert Werner","submitted_at":"2020-09-14T18:00:00Z","abstract_excerpt":"Recent X-ray observations have revealed remarkable correlations between the masses of central supermassive black holes (SMBHs) and the X-ray properties of the hot atmospheres permeating their host galaxies, thereby indicating the crucial role of the atmospheric gas in tracing SMBH growth in the high-mass regime. We examine this topic theoretically using the IllustrisTNG cosmological simulations and provide insights to the nature of this SMBH -- gaseous halo connection. By carrying out a mock X-ray analysis for a mass-selected sample of TNG100 simulated galaxies at $z=0$, we inspect the relatio"},"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":"2009.06634","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2020-09-14T18:00:00Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"5db3db133382131803d4791b3bb64469914f878ca0ca63c9b8cdf2069af22340","abstract_canon_sha256":"e48b5c96421bc41cd69e9765e32215d67b432f953fd256f9125ed7fd3eaa1ec5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:04:43.479994Z","signature_b64":"WoE3ksQCj51p0mogLj2+y2B6ek72nbrfdiadC/lI9qwm+ZVW9RwT0xSxt3IudnxblD0zJGkBAan5oX1LtwXXCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d8c3ae5c772a57f46063eb6747df8922fc118452ced19450e57485f0d673a9a3","last_reissued_at":"2026-07-05T02:04:43.479614Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:04:43.479614Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Annalisa Pillepich, Nhut Truong, Norbert Werner","submitted_at":"2020-09-14T18:00:00Z","abstract_excerpt":"Recent X-ray observations have revealed remarkable correlations between the masses of central supermassive black holes (SMBHs) and the X-ray properties of the hot atmospheres permeating their host galaxies, thereby indicating the crucial role of the atmospheric gas in tracing SMBH growth in the high-mass regime. We examine this topic theoretically using the IllustrisTNG cosmological simulations and provide insights to the nature of this SMBH -- gaseous halo connection. By carrying out a mock X-ray analysis for a mass-selected sample of TNG100 simulated galaxies at $z=0$, we inspect the relatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.06634","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/2009.06634/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":"2009.06634","created_at":"2026-07-05T02:04:43.479671+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.06634v2","created_at":"2026-07-05T02:04:43.479671+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.06634","created_at":"2026-07-05T02:04:43.479671+00:00"},{"alias_kind":"pith_short_12","alias_value":"3DB24XDXFJL7","created_at":"2026-07-05T02:04:43.479671+00:00"},{"alias_kind":"pith_short_16","alias_value":"3DB24XDXFJL7IYDD","created_at":"2026-07-05T02:04:43.479671+00:00"},{"alias_kind":"pith_short_8","alias_value":"3DB24XDX","created_at":"2026-07-05T02:04:43.479671+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.01820","citing_title":"The Cosmological analysis of X-ray cluster surveys VII. Bypassing scaling relations with Lagrangian Deep Learning and Simulation-based inference","ref_index":57,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL","json":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL.json","graph_json":"https://pith.science/api/pith-number/3DB24XDXFJL7IYDD5NTUPX4JEL/graph.json","events_json":"https://pith.science/api/pith-number/3DB24XDXFJL7IYDD5NTUPX4JEL/events.json","paper":"https://pith.science/paper/3DB24XDX"},"agent_actions":{"view_html":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL","download_json":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL.json","view_paper":"https://pith.science/paper/3DB24XDX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.06634&json=true","fetch_graph":"https://pith.science/api/pith-number/3DB24XDXFJL7IYDD5NTUPX4JEL/graph.json","fetch_events":"https://pith.science/api/pith-number/3DB24XDXFJL7IYDD5NTUPX4JEL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL/action/storage_attestation","attest_author":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL/action/author_attestation","sign_citation":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL/action/citation_signature","submit_replication":"https://pith.science/pith/3DB24XDXFJL7IYDD5NTUPX4JEL/action/replication_record"}},"created_at":"2026-07-05T02:04:43.479671+00:00","updated_at":"2026-07-05T02:04:43.479671+00:00"}