{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:SF34N6EOQJKGDHRFPRNLHESPNJ","short_pith_number":"pith:SF34N6EO","schema_version":"1.0","canonical_sha256":"9177c6f88e8254619e257c5ab3924f6a7408099ffe6e32cd7cc9c6ee1886f320","source":{"kind":"arxiv","id":"1007.5207","version":1},"attestation_state":"computed","paper":{"title":"Rotation Measures of Radio Sources in Hot Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Bonafede, F. Govoni, G. Giovannini, K. Dolag, L. Feretti, M. Murgia, S. Schindler, V. Vacca, W. Boschin","submitted_at":"2010-07-29T12:50:21Z","abstract_excerpt":"The goal of this work is to investigate the Faraday rotation measure (RM) of radio galaxies in hot galaxy clusters in order to establish a possible connection between the magnetic field strength and the gas temperature of the intracluster medium. We performed Very Large Array observations at 3.6 cm and 6 cm of two radio galaxies located in A401 and Ophiuchus, a radio galaxy in A2142, and a radio galaxy located in the background of A2065. All these galaxy clusters are characterized by high temperatures. We obtained detailed RM images at an angular resolution of 3'' for most of the observed radi"},"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":"1007.5207","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-07-29T12:50:21Z","cross_cats_sorted":[],"title_canon_sha256":"2506fe7c5d9458aa185cf4b6b9347c8c39cad9b59fd146496cecffc9e98a94dd","abstract_canon_sha256":"5e5180ea7793f727d1003023e325630c17ef5443ea4e036d41af48f459395196"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:01.354935Z","signature_b64":"D57uXCEcFUPjR8eN5MS5TqcKF0e8vt3LTnCYbimDpaw4VjsG3zNymLQvL3XXjGsHtgg5kOM5TpB3xQ0KLZrqBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9177c6f88e8254619e257c5ab3924f6a7408099ffe6e32cd7cc9c6ee1886f320","last_reissued_at":"2026-05-18T02:06:01.354230Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:01.354230Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rotation Measures of Radio Sources in Hot Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Bonafede, F. Govoni, G. Giovannini, K. Dolag, L. Feretti, M. Murgia, S. Schindler, V. Vacca, W. Boschin","submitted_at":"2010-07-29T12:50:21Z","abstract_excerpt":"The goal of this work is to investigate the Faraday rotation measure (RM) of radio galaxies in hot galaxy clusters in order to establish a possible connection between the magnetic field strength and the gas temperature of the intracluster medium. We performed Very Large Array observations at 3.6 cm and 6 cm of two radio galaxies located in A401 and Ophiuchus, a radio galaxy in A2142, and a radio galaxy located in the background of A2065. All these galaxy clusters are characterized by high temperatures. We obtained detailed RM images at an angular resolution of 3'' for most of the observed radi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1007.5207","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":""},"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":"1007.5207","created_at":"2026-05-18T02:06:01.354364+00:00"},{"alias_kind":"arxiv_version","alias_value":"1007.5207v1","created_at":"2026-05-18T02:06:01.354364+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1007.5207","created_at":"2026-05-18T02:06:01.354364+00:00"},{"alias_kind":"pith_short_12","alias_value":"SF34N6EOQJKG","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_16","alias_value":"SF34N6EOQJKGDHRF","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_8","alias_value":"SF34N6EO","created_at":"2026-05-18T12:26:13.927090+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/SF34N6EOQJKGDHRFPRNLHESPNJ","json":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ.json","graph_json":"https://pith.science/api/pith-number/SF34N6EOQJKGDHRFPRNLHESPNJ/graph.json","events_json":"https://pith.science/api/pith-number/SF34N6EOQJKGDHRFPRNLHESPNJ/events.json","paper":"https://pith.science/paper/SF34N6EO"},"agent_actions":{"view_html":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ","download_json":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ.json","view_paper":"https://pith.science/paper/SF34N6EO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1007.5207&json=true","fetch_graph":"https://pith.science/api/pith-number/SF34N6EOQJKGDHRFPRNLHESPNJ/graph.json","fetch_events":"https://pith.science/api/pith-number/SF34N6EOQJKGDHRFPRNLHESPNJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ/action/storage_attestation","attest_author":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ/action/author_attestation","sign_citation":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ/action/citation_signature","submit_replication":"https://pith.science/pith/SF34N6EOQJKGDHRFPRNLHESPNJ/action/replication_record"}},"created_at":"2026-05-18T02:06:01.354364+00:00","updated_at":"2026-05-18T02:06:01.354364+00:00"}