{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:YWNWLQD243DHSOUUNLRIUS2WFY","short_pith_number":"pith:YWNWLQD2","schema_version":"1.0","canonical_sha256":"c59b65c07ae6c6793a946ae28a4b562e19ec47dcb5233fb65ae3affded4d4e18","source":{"kind":"arxiv","id":"astro-ph/0612663","version":2},"attestation_state":"computed","paper":{"title":"Accurate Realizations of the Ionized Gas in Galaxy Clusters: Calibrating Feedback","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Jeremiah P. Ostriker, Jochen Weller, Laurie Shaw, Paul Bode","submitted_at":"2006-12-21T18:05:28Z","abstract_excerpt":"Using the full, three-dimensional potential of galaxy cluster halos (drawn from an N-body simulation of the current, most favored cosmology), the distribution of the X-ray emitting gas is found by assuming a polytropic equation of state and hydrostatic equilibrium, with constraints from conservation of energy and pressure balance at the cluster boundary. The resulting properties of the gas for these simulated redshift zero clusters (the temperature distribution, mass-temperature and luminosity-temperature relations, and the gas fraction) are compared with observations in the X-ray of nearby cl"},"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":"astro-ph/0612663","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-21T18:05:28Z","cross_cats_sorted":[],"title_canon_sha256":"7c74ddf26418de56545e2d6fb8c5ceac70b44525d18ed61416b4ceb3fbf0a5ba","abstract_canon_sha256":"0e28a9c81246756257a648c59baf63fdcf15b3c24dac84403634a444ad944dd6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:29:14.611848Z","signature_b64":"XYvf2TXCwxMYlS19Mqr+MJz7rTYYhmo5CQmNi11fIX3ZKCNhlVnoDCzG4UR6VD59Ri5cZLvbBi+3ioIbrOy0Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c59b65c07ae6c6793a946ae28a4b562e19ec47dcb5233fb65ae3affded4d4e18","last_reissued_at":"2026-05-18T04:29:14.611342Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:29:14.611342Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Accurate Realizations of the Ionized Gas in Galaxy Clusters: Calibrating Feedback","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Jeremiah P. Ostriker, Jochen Weller, Laurie Shaw, Paul Bode","submitted_at":"2006-12-21T18:05:28Z","abstract_excerpt":"Using the full, three-dimensional potential of galaxy cluster halos (drawn from an N-body simulation of the current, most favored cosmology), the distribution of the X-ray emitting gas is found by assuming a polytropic equation of state and hydrostatic equilibrium, with constraints from conservation of energy and pressure balance at the cluster boundary. The resulting properties of the gas for these simulated redshift zero clusters (the temperature distribution, mass-temperature and luminosity-temperature relations, and the gas fraction) are compared with observations in the X-ray of nearby cl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612663","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":""},"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":"astro-ph/0612663","created_at":"2026-05-18T04:29:14.611416+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0612663v2","created_at":"2026-05-18T04:29:14.611416+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0612663","created_at":"2026-05-18T04:29:14.611416+00:00"},{"alias_kind":"pith_short_12","alias_value":"YWNWLQD243DH","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_16","alias_value":"YWNWLQD243DHSOUU","created_at":"2026-05-18T12:25:54.717736+00:00"},{"alias_kind":"pith_short_8","alias_value":"YWNWLQD2","created_at":"2026-05-18T12:25:54.717736+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY","json":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY.json","graph_json":"https://pith.science/api/pith-number/YWNWLQD243DHSOUUNLRIUS2WFY/graph.json","events_json":"https://pith.science/api/pith-number/YWNWLQD243DHSOUUNLRIUS2WFY/events.json","paper":"https://pith.science/paper/YWNWLQD2"},"agent_actions":{"view_html":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY","download_json":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY.json","view_paper":"https://pith.science/paper/YWNWLQD2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0612663&json=true","fetch_graph":"https://pith.science/api/pith-number/YWNWLQD243DHSOUUNLRIUS2WFY/graph.json","fetch_events":"https://pith.science/api/pith-number/YWNWLQD243DHSOUUNLRIUS2WFY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY/action/storage_attestation","attest_author":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY/action/author_attestation","sign_citation":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY/action/citation_signature","submit_replication":"https://pith.science/pith/YWNWLQD243DHSOUUNLRIUS2WFY/action/replication_record"}},"created_at":"2026-05-18T04:29:14.611416+00:00","updated_at":"2026-05-18T04:29:14.611416+00:00"}