{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:I5C4I3CKMN3BBFJ4YQSXVSIEZH","short_pith_number":"pith:I5C4I3CK","schema_version":"1.0","canonical_sha256":"4745c46c4a637610953cc4257ac904c9f317c7d5bada8bc7b0610631b02c769c","source":{"kind":"arxiv","id":"1207.3735","version":1},"attestation_state":"computed","paper":{"title":"Simulating SZ intensity maps of giant AGN cocoons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Moraghan, D. A. Prokhorov, J. Silk, V. Antonuccio-Delogu","submitted_at":"2012-07-16T17:20:36Z","abstract_excerpt":"We perform relativistic hydrodynamic simulations of the formation and evolution of AGN cocoons produced by very light powerful jets. We calculate the intensity maps of the Sunyaev-Zel'dovich (SZ) effect at high frequencies for the simulated AGN cocoons using the relativistically correct Wright formalism. Our fully relativistic calculations demonstrate that the contribution from the high temperature gas (kb Te ~ 100 keV) to the SZ signal from AGN cocoons at high frequencies is stronger than that from the shocked ambient intercluster medium owing to the fact that the relativistic spectral functi"},"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":"1207.3735","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-07-16T17:20:36Z","cross_cats_sorted":[],"title_canon_sha256":"ba833759ce90ab5d6c7b4748eb13efbc06e23c6a60e84b4b684ebc12f125d017","abstract_canon_sha256":"64465bff0a984101bfcaf3a8ed0dac799a0ff7ed373ed00e7b0813609a35ef75"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:17.942757Z","signature_b64":"wRiL01/vwAeKIazlmXXieHT3PN2r+Ez4PMWbpcNJSx5cmvYRi3T0pDRBl3W+e0P7i4ByBTKods2b4UjDIf7OBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4745c46c4a637610953cc4257ac904c9f317c7d5bada8bc7b0610631b02c769c","last_reissued_at":"2026-05-18T01:56:17.942205Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:17.942205Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simulating SZ intensity maps of giant AGN cocoons","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Moraghan, D. A. Prokhorov, J. Silk, V. Antonuccio-Delogu","submitted_at":"2012-07-16T17:20:36Z","abstract_excerpt":"We perform relativistic hydrodynamic simulations of the formation and evolution of AGN cocoons produced by very light powerful jets. We calculate the intensity maps of the Sunyaev-Zel'dovich (SZ) effect at high frequencies for the simulated AGN cocoons using the relativistically correct Wright formalism. Our fully relativistic calculations demonstrate that the contribution from the high temperature gas (kb Te ~ 100 keV) to the SZ signal from AGN cocoons at high frequencies is stronger than that from the shocked ambient intercluster medium owing to the fact that the relativistic spectral functi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1207.3735","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":"1207.3735","created_at":"2026-05-18T01:56:17.942283+00:00"},{"alias_kind":"arxiv_version","alias_value":"1207.3735v1","created_at":"2026-05-18T01:56:17.942283+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1207.3735","created_at":"2026-05-18T01:56:17.942283+00:00"},{"alias_kind":"pith_short_12","alias_value":"I5C4I3CKMN3B","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_16","alias_value":"I5C4I3CKMN3BBFJ4","created_at":"2026-05-18T12:27:09.501522+00:00"},{"alias_kind":"pith_short_8","alias_value":"I5C4I3CK","created_at":"2026-05-18T12:27:09.501522+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/I5C4I3CKMN3BBFJ4YQSXVSIEZH","json":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH.json","graph_json":"https://pith.science/api/pith-number/I5C4I3CKMN3BBFJ4YQSXVSIEZH/graph.json","events_json":"https://pith.science/api/pith-number/I5C4I3CKMN3BBFJ4YQSXVSIEZH/events.json","paper":"https://pith.science/paper/I5C4I3CK"},"agent_actions":{"view_html":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH","download_json":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH.json","view_paper":"https://pith.science/paper/I5C4I3CK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1207.3735&json=true","fetch_graph":"https://pith.science/api/pith-number/I5C4I3CKMN3BBFJ4YQSXVSIEZH/graph.json","fetch_events":"https://pith.science/api/pith-number/I5C4I3CKMN3BBFJ4YQSXVSIEZH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH/action/storage_attestation","attest_author":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH/action/author_attestation","sign_citation":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH/action/citation_signature","submit_replication":"https://pith.science/pith/I5C4I3CKMN3BBFJ4YQSXVSIEZH/action/replication_record"}},"created_at":"2026-05-18T01:56:17.942283+00:00","updated_at":"2026-05-18T01:56:17.942283+00:00"}