{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:CP6HXKHBYWISYVEN4H3XYQ27LA","short_pith_number":"pith:CP6HXKHB","schema_version":"1.0","canonical_sha256":"13fc7ba8e1c5912c548de1f77c435f5803aee662edfc8898f7cac8f069872abb","source":{"kind":"arxiv","id":"1904.04199","version":1},"attestation_state":"computed","paper":{"title":"Constraining the Rotational Kinematic Sunyaev-Zel'dovich Effect in Massive Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Blake D. Sherwin, Eric J. Baxter, Srinivasan Raghunathan","submitted_at":"2019-04-08T17:17:42Z","abstract_excerpt":"We constrain the rotational kinematic Sunyaev-Zel'dovich (rkSZ) effect in Planck data using a sample of rotating galaxy clusters identified in the Sloan Digital Sky Survey (SDSS). We extract cluster-centered cutouts from Planck cosmic microwave background (CMB) maps that have been cleaned of thermal SZ signal. Using previous constraints on the cluster rotation vectors determined from the motions of galaxies, we fit for the amplitude of the rkSZ effect in the CMB cutouts, marginalizing over parameters describing the cluster electron distribution. We also employ an alternative, less model-depend"},"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":"1904.04199","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2019-04-08T17:17:42Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"70f7d5a9ae448b920e93219bde74b268d824e0bc0bbfbaf2157755b08be02e6e","abstract_canon_sha256":"1efe99ef7818f9f660786657a0d7e61a2b3f8ecaf992f753fcec55e3a50540d5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:04:03.109325Z","signature_b64":"MX69tuOYKw1w9jtJ1Qld4+82/cO1kEFJxqIlBlTP0jIahrCg2vM2zQWuYUZdpzs20D8umPeH/NXWstSiIc3tAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"13fc7ba8e1c5912c548de1f77c435f5803aee662edfc8898f7cac8f069872abb","last_reissued_at":"2026-07-05T02:04:03.108895Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:04:03.108895Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining the Rotational Kinematic Sunyaev-Zel'dovich Effect in Massive Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Blake D. Sherwin, Eric J. Baxter, Srinivasan Raghunathan","submitted_at":"2019-04-08T17:17:42Z","abstract_excerpt":"We constrain the rotational kinematic Sunyaev-Zel'dovich (rkSZ) effect in Planck data using a sample of rotating galaxy clusters identified in the Sloan Digital Sky Survey (SDSS). We extract cluster-centered cutouts from Planck cosmic microwave background (CMB) maps that have been cleaned of thermal SZ signal. Using previous constraints on the cluster rotation vectors determined from the motions of galaxies, we fit for the amplitude of the rkSZ effect in the CMB cutouts, marginalizing over parameters describing the cluster electron distribution. We also employ an alternative, less model-depend"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.04199","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1904.04199/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":"1904.04199","created_at":"2026-07-05T02:04:03.108952+00:00"},{"alias_kind":"arxiv_version","alias_value":"1904.04199v1","created_at":"2026-07-05T02:04:03.108952+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1904.04199","created_at":"2026-07-05T02:04:03.108952+00:00"},{"alias_kind":"pith_short_12","alias_value":"CP6HXKHBYWIS","created_at":"2026-07-05T02:04:03.108952+00:00"},{"alias_kind":"pith_short_16","alias_value":"CP6HXKHBYWISYVEN","created_at":"2026-07-05T02:04:03.108952+00:00"},{"alias_kind":"pith_short_8","alias_value":"CP6HXKHB","created_at":"2026-07-05T02:04:03.108952+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06659","citing_title":"The Treble Clef radio phoenix and its old nonthermal filaments","ref_index":288,"is_internal_anchor":true},{"citing_arxiv_id":"2605.15947","citing_title":"Dipoles for everyone: the pseudo-$C_\\ell$ approach to directional stacking","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA","json":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA.json","graph_json":"https://pith.science/api/pith-number/CP6HXKHBYWISYVEN4H3XYQ27LA/graph.json","events_json":"https://pith.science/api/pith-number/CP6HXKHBYWISYVEN4H3XYQ27LA/events.json","paper":"https://pith.science/paper/CP6HXKHB"},"agent_actions":{"view_html":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA","download_json":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA.json","view_paper":"https://pith.science/paper/CP6HXKHB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1904.04199&json=true","fetch_graph":"https://pith.science/api/pith-number/CP6HXKHBYWISYVEN4H3XYQ27LA/graph.json","fetch_events":"https://pith.science/api/pith-number/CP6HXKHBYWISYVEN4H3XYQ27LA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA/action/storage_attestation","attest_author":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA/action/author_attestation","sign_citation":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA/action/citation_signature","submit_replication":"https://pith.science/pith/CP6HXKHBYWISYVEN4H3XYQ27LA/action/replication_record"}},"created_at":"2026-07-05T02:04:03.108952+00:00","updated_at":"2026-07-05T02:04:03.108952+00:00"}