{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:BBOPCBCXJDCVFCR75M2ZH2HXUE","short_pith_number":"pith:BBOPCBCX","canonical_record":{"source":{"id":"1003.4256","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-03-22T19:55:49Z","cross_cats_sorted":[],"title_canon_sha256":"e6df2fa0597c2a01eaa2a0dd367113fbd59a72eaa9b09544228e000ab629e4fa","abstract_canon_sha256":"5f9adffe365eeb11199f8952413e787760fadc0b54b177d43bc2b12be7ed93b3"},"schema_version":"1.0"},"canonical_sha256":"085cf1045748c5528a3feb3593e8f7a10891c8d7dcaaacca69506e5ef890d3d2","source":{"kind":"arxiv","id":"1003.4256","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1003.4256","created_at":"2026-05-18T02:08:24Z"},{"alias_kind":"arxiv_version","alias_value":"1003.4256v2","created_at":"2026-05-18T02:08:24Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1003.4256","created_at":"2026-05-18T02:08:24Z"},{"alias_kind":"pith_short_12","alias_value":"BBOPCBCXJDCV","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_16","alias_value":"BBOPCBCXJDCVFCR7","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_8","alias_value":"BBOPCBCX","created_at":"2026-05-18T12:26:05Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:BBOPCBCXJDCVFCR75M2ZH2HXUE","target":"record","payload":{"canonical_record":{"source":{"id":"1003.4256","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-03-22T19:55:49Z","cross_cats_sorted":[],"title_canon_sha256":"e6df2fa0597c2a01eaa2a0dd367113fbd59a72eaa9b09544228e000ab629e4fa","abstract_canon_sha256":"5f9adffe365eeb11199f8952413e787760fadc0b54b177d43bc2b12be7ed93b3"},"schema_version":"1.0"},"canonical_sha256":"085cf1045748c5528a3feb3593e8f7a10891c8d7dcaaacca69506e5ef890d3d2","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:08:24.504602Z","signature_b64":"RwR5iPfz5GYa48OT2C0dNrPyHZ6PYLmGclBQJM7AbcrS3IJXwoN7Vvu65tUJyZlY4ZGb7oNEd8K4PEBj30X5BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"085cf1045748c5528a3feb3593e8f7a10891c8d7dcaaacca69506e5ef890d3d2","last_reissued_at":"2026-05-18T02:08:24.503871Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:08:24.503871Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1003.4256","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:08:24Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3s6ss9VlfVWzoFeypPdUpLsqKDiECpjiLBjS5bJU/O8q5mKhSSJniX4bsI8iW75S/hOB9z+vK+GNpezDgR+jDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T18:45:52.894581Z"},"content_sha256":"9f6b2081b75d6bdc6bae5a0c231fb15b0665318ffe8bc9f2fb4c723da1de46ba","schema_version":"1.0","event_id":"sha256:9f6b2081b75d6bdc6bae5a0c231fb15b0665318ffe8bc9f2fb4c723da1de46ba"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:BBOPCBCXJDCVFCR75M2ZH2HXUE","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Simulations of the Sunyaev-Zel'dovich Power Spectrum with AGN Feedback","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"CITA), C. Pfrommer (CITA), D. Sijacki (Cambridge), J. L. Sievers (CITA), J. R. Bond (CITA), N. Battaglia (U of Toronto","submitted_at":"2010-03-22T19:55:49Z","abstract_excerpt":"We explore how radiative cooling, supernova feedback, cosmic rays and a new model of the energetic feedback from active galactic nuclei (AGN) affect the thermal and kinetic Sunyaev-Zel'dovich (SZ) power spectra. To do this, we use a suite of hydrodynamical TreePM-SPH simulations of the cosmic web in large periodic boxes and tailored higher resolution simulations of individual galaxy clusters. Our AGN feedback simulations match the recent universal pressure profile and cluster mass scaling relations of the REXCESS X-ray cluster sample better than previous analytical or numerical approaches. For"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.4256","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:08:24Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5aEfInJSMeDKAuXf8RfEGeJTWUzKngDkLQS9Xr2Tc0NncUr4iDkzIMp2UoR92zXOpATiR/WO3pMO0d/b810bAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T18:45:52.894942Z"},"content_sha256":"8837df30958f2eb5b968ee23a24ab09a2fc486aef2ea70afc47af79cd7889c34","schema_version":"1.0","event_id":"sha256:8837df30958f2eb5b968ee23a24ab09a2fc486aef2ea70afc47af79cd7889c34"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/BBOPCBCXJDCVFCR75M2ZH2HXUE/bundle.json","state_url":"https://pith.science/pith/BBOPCBCXJDCVFCR75M2ZH2HXUE/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/BBOPCBCXJDCVFCR75M2ZH2HXUE/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-02T18:45:52Z","links":{"resolver":"https://pith.science/pith/BBOPCBCXJDCVFCR75M2ZH2HXUE","bundle":"https://pith.science/pith/BBOPCBCXJDCVFCR75M2ZH2HXUE/bundle.json","state":"https://pith.science/pith/BBOPCBCXJDCVFCR75M2ZH2HXUE/state.json","well_known_bundle":"https://pith.science/.well-known/pith/BBOPCBCXJDCVFCR75M2ZH2HXUE/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:BBOPCBCXJDCVFCR75M2ZH2HXUE","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"5f9adffe365eeb11199f8952413e787760fadc0b54b177d43bc2b12be7ed93b3","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-03-22T19:55:49Z","title_canon_sha256":"e6df2fa0597c2a01eaa2a0dd367113fbd59a72eaa9b09544228e000ab629e4fa"},"schema_version":"1.0","source":{"id":"1003.4256","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1003.4256","created_at":"2026-05-18T02:08:24Z"},{"alias_kind":"arxiv_version","alias_value":"1003.4256v2","created_at":"2026-05-18T02:08:24Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1003.4256","created_at":"2026-05-18T02:08:24Z"},{"alias_kind":"pith_short_12","alias_value":"BBOPCBCXJDCV","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_16","alias_value":"BBOPCBCXJDCVFCR7","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_8","alias_value":"BBOPCBCX","created_at":"2026-05-18T12:26:05Z"}],"graph_snapshots":[{"event_id":"sha256:8837df30958f2eb5b968ee23a24ab09a2fc486aef2ea70afc47af79cd7889c34","target":"graph","created_at":"2026-05-18T02:08:24Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We explore how radiative cooling, supernova feedback, cosmic rays and a new model of the energetic feedback from active galactic nuclei (AGN) affect the thermal and kinetic Sunyaev-Zel'dovich (SZ) power spectra. To do this, we use a suite of hydrodynamical TreePM-SPH simulations of the cosmic web in large periodic boxes and tailored higher resolution simulations of individual galaxy clusters. Our AGN feedback simulations match the recent universal pressure profile and cluster mass scaling relations of the REXCESS X-ray cluster sample better than previous analytical or numerical approaches. For","authors_text":"CITA), C. Pfrommer (CITA), D. Sijacki (Cambridge), J. L. Sievers (CITA), J. R. Bond (CITA), N. Battaglia (U of Toronto","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-03-22T19:55:49Z","title":"Simulations of the Sunyaev-Zel'dovich Power Spectrum with AGN Feedback"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.4256","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:9f6b2081b75d6bdc6bae5a0c231fb15b0665318ffe8bc9f2fb4c723da1de46ba","target":"record","created_at":"2026-05-18T02:08:24Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"5f9adffe365eeb11199f8952413e787760fadc0b54b177d43bc2b12be7ed93b3","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-03-22T19:55:49Z","title_canon_sha256":"e6df2fa0597c2a01eaa2a0dd367113fbd59a72eaa9b09544228e000ab629e4fa"},"schema_version":"1.0","source":{"id":"1003.4256","kind":"arxiv","version":2}},"canonical_sha256":"085cf1045748c5528a3feb3593e8f7a10891c8d7dcaaacca69506e5ef890d3d2","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"085cf1045748c5528a3feb3593e8f7a10891c8d7dcaaacca69506e5ef890d3d2","first_computed_at":"2026-05-18T02:08:24.503871Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:08:24.503871Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"RwR5iPfz5GYa48OT2C0dNrPyHZ6PYLmGclBQJM7AbcrS3IJXwoN7Vvu65tUJyZlY4ZGb7oNEd8K4PEBj30X5BQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:08:24.504602Z","signed_message":"canonical_sha256_bytes"},"source_id":"1003.4256","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:9f6b2081b75d6bdc6bae5a0c231fb15b0665318ffe8bc9f2fb4c723da1de46ba","sha256:8837df30958f2eb5b968ee23a24ab09a2fc486aef2ea70afc47af79cd7889c34"],"state_sha256":"83e9f68a60fd78188252a7428333f2de71aab3dff521890ac00514ef9cef7075"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"h5v5tAnbgA1EXYAg9TBvyiBGPe3t82+WTpg6bMX78vBY5aE8WSpyq3G3DjVBNZl2vV8jz5OQ6s6SpMO2E75JCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T18:45:52.896950Z","bundle_sha256":"be68aff8c10b7a44220425d162036af9f4a3be589d28d1f2236ca481c9cfd926"}}