{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:IEDZUF6YN6YFIOL6FXY4PZ23AC","short_pith_number":"pith:IEDZUF6Y","schema_version":"1.0","canonical_sha256":"41079a17d86fb054397e2df1c7e75b008e6b85502ca25e8d2cd08a758b9c7a13","source":{"kind":"arxiv","id":"astro-ph/0609480","version":1},"attestation_state":"computed","paper":{"title":"Temperature profiles of a representative sample of nearby X-ray galaxy clusters","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Finoguenov, G.W. Pratt (MPE Garching), H. Boehringer, J.H. Croston, M. Arnaud, R.F. Temple, S. Borgani","submitted_at":"2006-09-18T12:38:13Z","abstract_excerpt":"A study of the structural and scaling properties of the temperature distribution of the hot, X-ray emitting intra-cluster medium of galaxy clusters, and its dependence on dynamical state, can give insights into the physical processes governing the formation and evolution of structure. We analyse the X-ray temperature profiles from XMM-Newton observations of 15 nearby (z < 0.2) clusters, drawn from a statistically representative sample. The clusters cover a temperature range from 2.5 keV to 8.5 keV, and present a variety of X-ray morphologies. We derive accurate projected temperature profiles t"},"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/0609480","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-09-18T12:38:13Z","cross_cats_sorted":[],"title_canon_sha256":"0f4de2ce325fbbf16bd98b9f646f132af85481c7d70c7451c0832d56b2dd469a","abstract_canon_sha256":"b99fab3c9a13e8efd0f77c0db77f9c34fa4dd513e65d498c0df8c6e91b80d8ad"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:59:25.167631Z","signature_b64":"pqyfvaiN8WHiqzwRzm61PoWK5EYqMcwtrnTR248oNf5jWDjAsVrEvI1h89hT54aB2oemuzP6Hy/f3MfqUVAXAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"41079a17d86fb054397e2df1c7e75b008e6b85502ca25e8d2cd08a758b9c7a13","last_reissued_at":"2026-07-04T16:59:25.167272Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:59:25.167272Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Temperature profiles of a representative sample of nearby X-ray galaxy clusters","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Finoguenov, G.W. Pratt (MPE Garching), H. Boehringer, J.H. Croston, M. Arnaud, R.F. Temple, S. Borgani","submitted_at":"2006-09-18T12:38:13Z","abstract_excerpt":"A study of the structural and scaling properties of the temperature distribution of the hot, X-ray emitting intra-cluster medium of galaxy clusters, and its dependence on dynamical state, can give insights into the physical processes governing the formation and evolution of structure. We analyse the X-ray temperature profiles from XMM-Newton observations of 15 nearby (z < 0.2) clusters, drawn from a statistically representative sample. The clusters cover a temperature range from 2.5 keV to 8.5 keV, and present a variety of X-ray morphologies. We derive accurate projected temperature profiles t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0609480","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/astro-ph/0609480/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":"astro-ph/0609480","created_at":"2026-07-04T16:59:25.167337+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0609480v1","created_at":"2026-07-04T16:59:25.167337+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0609480","created_at":"2026-07-04T16:59:25.167337+00:00"},{"alias_kind":"pith_short_12","alias_value":"IEDZUF6YN6YF","created_at":"2026-07-04T16:59:25.167337+00:00"},{"alias_kind":"pith_short_16","alias_value":"IEDZUF6YN6YFIOL6","created_at":"2026-07-04T16:59:25.167337+00:00"},{"alias_kind":"pith_short_8","alias_value":"IEDZUF6Y","created_at":"2026-07-04T16:59:25.167337+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/IEDZUF6YN6YFIOL6FXY4PZ23AC","json":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC.json","graph_json":"https://pith.science/api/pith-number/IEDZUF6YN6YFIOL6FXY4PZ23AC/graph.json","events_json":"https://pith.science/api/pith-number/IEDZUF6YN6YFIOL6FXY4PZ23AC/events.json","paper":"https://pith.science/paper/IEDZUF6Y"},"agent_actions":{"view_html":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC","download_json":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC.json","view_paper":"https://pith.science/paper/IEDZUF6Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0609480&json=true","fetch_graph":"https://pith.science/api/pith-number/IEDZUF6YN6YFIOL6FXY4PZ23AC/graph.json","fetch_events":"https://pith.science/api/pith-number/IEDZUF6YN6YFIOL6FXY4PZ23AC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC/action/storage_attestation","attest_author":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC/action/author_attestation","sign_citation":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC/action/citation_signature","submit_replication":"https://pith.science/pith/IEDZUF6YN6YFIOL6FXY4PZ23AC/action/replication_record"}},"created_at":"2026-07-04T16:59:25.167337+00:00","updated_at":"2026-07-04T16:59:25.167337+00:00"}