{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:JGYRGCZLTKVTDWTXM5KVCYAJMK","short_pith_number":"pith:JGYRGCZL","schema_version":"1.0","canonical_sha256":"49b1130b2b9aab31da7767555160096284a9294135bd92d4dbeee99e535d1cc1","source":{"kind":"arxiv","id":"1701.03791","version":2},"attestation_state":"computed","paper":{"title":"Deep 230-470 MHz VLA Observations of the mini-halo in the Perseus Cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. C. Fabian, G. B. Taylor, H. T. Intema, J. Hlavacek-Larrondo, J. S. Sanders, K. M. Blundell, M. Gendron-Marsolais, R. J. van Weeren, T. Clarke","submitted_at":"2017-01-13T19:00:01Z","abstract_excerpt":"We present a low-frequency view of the Perseus cluster with new observations from the Karl G. Jansky Very Large Array (JVLA) at 230-470 MHz. The data reveal a multitude of new structures associated with the mini-halo. The mini-halo seems to be influenced both by the AGN activity as well as by the sloshing motion of the cool core cluster's gas. In addition, it has a filamentary structure similar to that seen in radio relics found in merging clusters. We present a detailed description of the data reduction and imaging process of the dataset. The depth and resolution of the observations allow us "},"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":"1701.03791","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-01-13T19:00:01Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"c3c2389b6e5e02a5fcd40769001307634cfdf2ce34cf603c8bfd8c96401877d7","abstract_canon_sha256":"9b07f111e824553e5cd780f663c57f59cb0d3218256c8edfbbbe5cc7ad8b9abf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:42:23.582853Z","signature_b64":"ph8mmibTXqPruKVoE84zn7VmvYQa+GdYZcenkgPK2KN/eD5UaYFBx7C0E6H1TsCNkIFIH9Ua7AJzox+JAxNvCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"49b1130b2b9aab31da7767555160096284a9294135bd92d4dbeee99e535d1cc1","last_reissued_at":"2026-05-18T00:42:23.582340Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:42:23.582340Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Deep 230-470 MHz VLA Observations of the mini-halo in the Perseus Cluster","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"A. C. Fabian, G. B. Taylor, H. T. Intema, J. Hlavacek-Larrondo, J. S. Sanders, K. M. Blundell, M. Gendron-Marsolais, R. J. van Weeren, T. Clarke","submitted_at":"2017-01-13T19:00:01Z","abstract_excerpt":"We present a low-frequency view of the Perseus cluster with new observations from the Karl G. Jansky Very Large Array (JVLA) at 230-470 MHz. The data reveal a multitude of new structures associated with the mini-halo. The mini-halo seems to be influenced both by the AGN activity as well as by the sloshing motion of the cool core cluster's gas. In addition, it has a filamentary structure similar to that seen in radio relics found in merging clusters. We present a detailed description of the data reduction and imaging process of the dataset. The depth and resolution of the observations allow us "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.03791","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":"1701.03791","created_at":"2026-05-18T00:42:23.582425+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.03791v2","created_at":"2026-05-18T00:42:23.582425+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.03791","created_at":"2026-05-18T00:42:23.582425+00:00"},{"alias_kind":"pith_short_12","alias_value":"JGYRGCZLTKVT","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_16","alias_value":"JGYRGCZLTKVTDWTX","created_at":"2026-05-18T12:31:24.725408+00:00"},{"alias_kind":"pith_short_8","alias_value":"JGYRGCZL","created_at":"2026-05-18T12:31:24.725408+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/JGYRGCZLTKVTDWTXM5KVCYAJMK","json":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK.json","graph_json":"https://pith.science/api/pith-number/JGYRGCZLTKVTDWTXM5KVCYAJMK/graph.json","events_json":"https://pith.science/api/pith-number/JGYRGCZLTKVTDWTXM5KVCYAJMK/events.json","paper":"https://pith.science/paper/JGYRGCZL"},"agent_actions":{"view_html":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK","download_json":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK.json","view_paper":"https://pith.science/paper/JGYRGCZL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.03791&json=true","fetch_graph":"https://pith.science/api/pith-number/JGYRGCZLTKVTDWTXM5KVCYAJMK/graph.json","fetch_events":"https://pith.science/api/pith-number/JGYRGCZLTKVTDWTXM5KVCYAJMK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK/action/storage_attestation","attest_author":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK/action/author_attestation","sign_citation":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK/action/citation_signature","submit_replication":"https://pith.science/pith/JGYRGCZLTKVTDWTXM5KVCYAJMK/action/replication_record"}},"created_at":"2026-05-18T00:42:23.582425+00:00","updated_at":"2026-05-18T00:42:23.582425+00:00"}