{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:UGSYZ3GPTVWVIXNYKQG2EBYKMC","short_pith_number":"pith:UGSYZ3GP","schema_version":"1.0","canonical_sha256":"a1a58ceccf9d6d545db8540da2070a60bf862d794340a3065a5b7cf6b4358d7a","source":{"kind":"arxiv","id":"1612.06296","version":2},"attestation_state":"computed","paper":{"title":"Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Bjoern Soergel, Debora Sijacki, Ewald Puchwein, George Efstathiou, Tommaso Giannantonio","submitted_at":"2016-12-19T18:02:14Z","abstract_excerpt":"We derive constraints on feedback by active galactic nuclei (AGN) by setting limits on their thermal Sunyaev-Zel'dovich (SZ) imprint on the cosmic microwave background (CMB). The amplitude of any SZ signature is small and degenerate with the poorly known sub-mm spectral energy distribution of the AGN host galaxy and other unresolved dusty sources along the line of sight. Here we break this degeneracy by combining microwave and sub-mm data from Planck with all-sky far-infrared maps from the AKARI satellite. We first test our measurement pipeline using the Sloan Digital Sky Survey (SDSS) redMaPP"},"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":"1612.06296","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-12-19T18:02:14Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"8e878fb4ca5fd75eba4736eedd4fe83233470f7e5439bd3981ba1d90ab4682c2","abstract_canon_sha256":"f6514e6811557a8ec8aa10ee919ef6ee390b1d3d38e4313feecb69430fcbcccf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:45:06.278196Z","signature_b64":"umTNGkW9N4Hd/GJNUlPrdYUfE9nwgTalXb7KjocnQa6H/Lh0VzWkafPdPzNHVIK1iimMLNqI7oAOZxGfpYRGAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a1a58ceccf9d6d545db8540da2070a60bf862d794340a3065a5b7cf6b4358d7a","last_reissued_at":"2026-05-18T00:45:06.277727Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:45:06.277727Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Bjoern Soergel, Debora Sijacki, Ewald Puchwein, George Efstathiou, Tommaso Giannantonio","submitted_at":"2016-12-19T18:02:14Z","abstract_excerpt":"We derive constraints on feedback by active galactic nuclei (AGN) by setting limits on their thermal Sunyaev-Zel'dovich (SZ) imprint on the cosmic microwave background (CMB). The amplitude of any SZ signature is small and degenerate with the poorly known sub-mm spectral energy distribution of the AGN host galaxy and other unresolved dusty sources along the line of sight. Here we break this degeneracy by combining microwave and sub-mm data from Planck with all-sky far-infrared maps from the AKARI satellite. We first test our measurement pipeline using the Sloan Digital Sky Survey (SDSS) redMaPP"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.06296","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":"1612.06296","created_at":"2026-05-18T00:45:06.277787+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.06296v2","created_at":"2026-05-18T00:45:06.277787+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.06296","created_at":"2026-05-18T00:45:06.277787+00:00"},{"alias_kind":"pith_short_12","alias_value":"UGSYZ3GPTVWV","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_16","alias_value":"UGSYZ3GPTVWVIXNY","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_8","alias_value":"UGSYZ3GP","created_at":"2026-05-18T12:30:46.583412+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/UGSYZ3GPTVWVIXNYKQG2EBYKMC","json":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC.json","graph_json":"https://pith.science/api/pith-number/UGSYZ3GPTVWVIXNYKQG2EBYKMC/graph.json","events_json":"https://pith.science/api/pith-number/UGSYZ3GPTVWVIXNYKQG2EBYKMC/events.json","paper":"https://pith.science/paper/UGSYZ3GP"},"agent_actions":{"view_html":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC","download_json":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC.json","view_paper":"https://pith.science/paper/UGSYZ3GP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.06296&json=true","fetch_graph":"https://pith.science/api/pith-number/UGSYZ3GPTVWVIXNYKQG2EBYKMC/graph.json","fetch_events":"https://pith.science/api/pith-number/UGSYZ3GPTVWVIXNYKQG2EBYKMC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC/action/storage_attestation","attest_author":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC/action/author_attestation","sign_citation":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC/action/citation_signature","submit_replication":"https://pith.science/pith/UGSYZ3GPTVWVIXNYKQG2EBYKMC/action/replication_record"}},"created_at":"2026-05-18T00:45:06.277787+00:00","updated_at":"2026-05-18T00:45:06.277787+00:00"}