{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:IXMV3SMGBP6VVHTNQHF3HUCCZC","short_pith_number":"pith:IXMV3SMG","schema_version":"1.0","canonical_sha256":"45d95dc9860bfd5a9e6d81cbb3d042c89cfa6d4d05cdd90dda3750db185c26ed","source":{"kind":"arxiv","id":"2503.08840","version":2},"attestation_state":"computed","paper":{"title":"Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bonafede, A. Drabent, A. M. Hopkins, B. S. Koribalski, C. J. Riseley, C. Pfrommer, C. S. Anderson, D. J. Bomans, E. Carretti, E. O'Sullivan, F. Gastaldello, F. Loi, H. R. M. Zovaro, J. West, K. Ross, K. Rubinur, L. Lovisari, L. Rudnick, M. Brienza, M. Ruszkowski, M. S. de Villiers, Prasanta K. Nayak, R. Santra, S. Giacintucci, S. W. Duchesne, T. Akahori, T. Vernstrom, T. W. Shimwell, W. Raja","submitted_at":"2025-03-11T19:22:42Z","abstract_excerpt":"In the context of the life cycle and evolution of active galactic nuclei (AGN), the environment plays an important role. In particular, the over-dense environments of galaxy groups, where dynamical interactions and bulk motions have significant impact, offer an excellent but under-explored window into the life cycles of AGN and the processes that shape the evolution of relativistic plasma. Pilot Survey observations with the Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) survey recovered diffuse emission associated with the nearby (z = 0.0228) galaxy"},"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":"2503.08840","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-03-11T19:22:42Z","cross_cats_sorted":[],"title_canon_sha256":"5a196260139c21af0d5808f252b3f760ccaf74a16e89bf227fa1594549a7fb1f","abstract_canon_sha256":"870f11475844d9130179c63f34a0cf348c8d476582382eb99a692fa561a54688"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:59:07.016774Z","signature_b64":"A0nIRomFqT2JyJDe5nHhb+o8EYeZAGfCTAEbYucR9/2mVg+sIXGCHWAT8aVaoS1LxHjFMygLOfJl8K733kUGAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"45d95dc9860bfd5a9e6d81cbb3d042c89cfa6d4d05cdd90dda3750db185c26ed","last_reissued_at":"2026-07-05T10:59:07.016258Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:59:07.016258Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bonafede, A. Drabent, A. M. Hopkins, B. S. Koribalski, C. J. Riseley, C. Pfrommer, C. S. Anderson, D. J. Bomans, E. Carretti, E. O'Sullivan, F. Gastaldello, F. Loi, H. R. M. Zovaro, J. West, K. Ross, K. Rubinur, L. Lovisari, L. Rudnick, M. Brienza, M. Ruszkowski, M. S. de Villiers, Prasanta K. Nayak, R. Santra, S. Giacintucci, S. W. Duchesne, T. Akahori, T. Vernstrom, T. W. Shimwell, W. Raja","submitted_at":"2025-03-11T19:22:42Z","abstract_excerpt":"In the context of the life cycle and evolution of active galactic nuclei (AGN), the environment plays an important role. In particular, the over-dense environments of galaxy groups, where dynamical interactions and bulk motions have significant impact, offer an excellent but under-explored window into the life cycles of AGN and the processes that shape the evolution of relativistic plasma. Pilot Survey observations with the Australian Square Kilometre Array Pathfinder (ASKAP) Evolutionary Map of the Universe (EMU) survey recovered diffuse emission associated with the nearby (z = 0.0228) galaxy"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.08840","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/2503.08840/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":"2503.08840","created_at":"2026-07-05T10:59:07.016324+00:00"},{"alias_kind":"arxiv_version","alias_value":"2503.08840v2","created_at":"2026-07-05T10:59:07.016324+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.08840","created_at":"2026-07-05T10:59:07.016324+00:00"},{"alias_kind":"pith_short_12","alias_value":"IXMV3SMGBP6V","created_at":"2026-07-05T10:59:07.016324+00:00"},{"alias_kind":"pith_short_16","alias_value":"IXMV3SMGBP6VVHTN","created_at":"2026-07-05T10:59:07.016324+00:00"},{"alias_kind":"pith_short_8","alias_value":"IXMV3SMG","created_at":"2026-07-05T10:59:07.016324+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/IXMV3SMGBP6VVHTNQHF3HUCCZC","json":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC.json","graph_json":"https://pith.science/api/pith-number/IXMV3SMGBP6VVHTNQHF3HUCCZC/graph.json","events_json":"https://pith.science/api/pith-number/IXMV3SMGBP6VVHTNQHF3HUCCZC/events.json","paper":"https://pith.science/paper/IXMV3SMG"},"agent_actions":{"view_html":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC","download_json":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC.json","view_paper":"https://pith.science/paper/IXMV3SMG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2503.08840&json=true","fetch_graph":"https://pith.science/api/pith-number/IXMV3SMGBP6VVHTNQHF3HUCCZC/graph.json","fetch_events":"https://pith.science/api/pith-number/IXMV3SMGBP6VVHTNQHF3HUCCZC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC/action/storage_attestation","attest_author":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC/action/author_attestation","sign_citation":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC/action/citation_signature","submit_replication":"https://pith.science/pith/IXMV3SMGBP6VVHTNQHF3HUCCZC/action/replication_record"}},"created_at":"2026-07-05T10:59:07.016324+00:00","updated_at":"2026-07-05T10:59:07.016324+00:00"}