{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:WXTY4OITT7SOHUIBZGOEW5QLWH","short_pith_number":"pith:WXTY4OIT","schema_version":"1.0","canonical_sha256":"b5e78e39139fe4e3d101c99c4b760bb1e1f4890baee2040eac5f4aea189bf5e7","source":{"kind":"arxiv","id":"1710.06796","version":1},"attestation_state":"computed","paper":{"title":"Gentle re-energisation of electrons in merging galaxy clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"A. Bonafede, F. De Gasperin, G. Brunetti, H. J. A. Rottgering, H. T. Intema, M. Bruggen, R. J. van Weeren, T. A. Ensslin, T. W. Shimwell","submitted_at":"2017-10-18T15:41:32Z","abstract_excerpt":"Galaxy clusters are the most massive constituents of the large-scale structure of the Universe. While the hot thermal gas that pervades galaxy clusters is relatively well understood through observations with X-ray satellites, our understanding of the non-thermal part of the intra-cluster medium remains incomplete. With LOFAR and GMRT observations, we have identified a phenomenon that can be unveiled only at extremely low radio-frequencies and offers new insights into the non-thermal component. We propose that the interplay between radio-emitting plasma and the perturbed intra-cluster medium ca"},"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":"1710.06796","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-10-18T15:41:32Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"54801f3c01d3afcff84411c641f744aa681ba5a09a064a4d5e1f6e9aa9172efb","abstract_canon_sha256":"1b67ce2614c4d6b9aceedb3bf8a08a848bd6382e44314608635422708b681d6e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:32:32.120111Z","signature_b64":"CNJNwa3WPKenZMMyMSOBOphkOMgx2FkFWHJ9ZzGkL0t7jb+CFc+xlY6vZUIyWn6rKQzZwo84DyfBPqBYwtHsAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b5e78e39139fe4e3d101c99c4b760bb1e1f4890baee2040eac5f4aea189bf5e7","last_reissued_at":"2026-05-18T00:32:32.119402Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:32:32.119402Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gentle re-energisation of electrons in merging galaxy clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"A. Bonafede, F. De Gasperin, G. Brunetti, H. J. A. Rottgering, H. T. Intema, M. Bruggen, R. J. van Weeren, T. A. Ensslin, T. W. Shimwell","submitted_at":"2017-10-18T15:41:32Z","abstract_excerpt":"Galaxy clusters are the most massive constituents of the large-scale structure of the Universe. While the hot thermal gas that pervades galaxy clusters is relatively well understood through observations with X-ray satellites, our understanding of the non-thermal part of the intra-cluster medium remains incomplete. With LOFAR and GMRT observations, we have identified a phenomenon that can be unveiled only at extremely low radio-frequencies and offers new insights into the non-thermal component. We propose that the interplay between radio-emitting plasma and the perturbed intra-cluster medium ca"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1710.06796","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":"1710.06796","created_at":"2026-05-18T00:32:32.119518+00:00"},{"alias_kind":"arxiv_version","alias_value":"1710.06796v1","created_at":"2026-05-18T00:32:32.119518+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1710.06796","created_at":"2026-05-18T00:32:32.119518+00:00"},{"alias_kind":"pith_short_12","alias_value":"WXTY4OITT7SO","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_16","alias_value":"WXTY4OITT7SOHUIB","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_8","alias_value":"WXTY4OIT","created_at":"2026-05-18T12:31:53.515858+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/WXTY4OITT7SOHUIBZGOEW5QLWH","json":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH.json","graph_json":"https://pith.science/api/pith-number/WXTY4OITT7SOHUIBZGOEW5QLWH/graph.json","events_json":"https://pith.science/api/pith-number/WXTY4OITT7SOHUIBZGOEW5QLWH/events.json","paper":"https://pith.science/paper/WXTY4OIT"},"agent_actions":{"view_html":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH","download_json":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH.json","view_paper":"https://pith.science/paper/WXTY4OIT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1710.06796&json=true","fetch_graph":"https://pith.science/api/pith-number/WXTY4OITT7SOHUIBZGOEW5QLWH/graph.json","fetch_events":"https://pith.science/api/pith-number/WXTY4OITT7SOHUIBZGOEW5QLWH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH/action/storage_attestation","attest_author":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH/action/author_attestation","sign_citation":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH/action/citation_signature","submit_replication":"https://pith.science/pith/WXTY4OITT7SOHUIBZGOEW5QLWH/action/replication_record"}},"created_at":"2026-05-18T00:32:32.119518+00:00","updated_at":"2026-05-18T00:32:32.119518+00:00"}