{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:QEPW7MWOLA5EABOHRC7ZKNQMOV","short_pith_number":"pith:QEPW7MWO","schema_version":"1.0","canonical_sha256":"811f6fb2ce583a4005c788bf95360c754213c08c085b15ad20485f29c62936c1","source":{"kind":"arxiv","id":"1812.06926","version":2},"attestation_state":"computed","paper":{"title":"Imaging the Thermal and Kinematic Sunyaev-Zel'dovich Effect Signals in a Sample of Ten Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adi Zitrin, Alfredo Monta\\~na, Daisuke Nagai, David Hughes, David S\\'anchez, Erik D. Reese, Grant W. Wilson, Jack Sayers, John ZuHone, Michael Zemcov, Nath\\'alia Cibirka, Sunil Golwala, Tony Mroczkowski","submitted_at":"2018-12-17T17:59:28Z","abstract_excerpt":"We have imaged the Sunyaev-Zel'dovich (SZ) effect signals at 140 and 270 GHz towards ten galaxy clusters with Bolocam and AzTEC/ASTE. We also used Planck data to constrain the signal at large angular scales, Herschel-SPIRE images to subtract the brightest galaxies that comprise the cosmic infrared background (CIB), Chandra imaging to map the electron temperature $T_e$ of the intra-cluster medium (ICM), and HST imaging to derive models of each galaxy cluster's mass density. The galaxy clusters gravitationally lens the background CIB, which produced an on-average reduction in brightness towards "},"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":"1812.06926","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-12-17T17:59:28Z","cross_cats_sorted":[],"title_canon_sha256":"18644ec54b4d7ca122b013d2815a87090fc8c026768567e5ff23fe4b1472c48c","abstract_canon_sha256":"4b8c694f683b94cbad4557a25f1bdd462c5e1524b2f3f02a786f051a69105ca4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:50:13.815933Z","signature_b64":"WYrJD6A1y3XSbvqa6mUkQGXgS8cXvdILUFkgmNY5rfNjZmJT89vZ0oG2xl3I95JMzzreKHHgGkRMVl6pkBCuDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"811f6fb2ce583a4005c788bf95360c754213c08c085b15ad20485f29c62936c1","last_reissued_at":"2026-07-04T23:50:13.815476Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:50:13.815476Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Imaging the Thermal and Kinematic Sunyaev-Zel'dovich Effect Signals in a Sample of Ten Massive Galaxy Clusters: Constraints on Internal Velocity Structures and Bulk Velocities","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adi Zitrin, Alfredo Monta\\~na, Daisuke Nagai, David Hughes, David S\\'anchez, Erik D. Reese, Grant W. Wilson, Jack Sayers, John ZuHone, Michael Zemcov, Nath\\'alia Cibirka, Sunil Golwala, Tony Mroczkowski","submitted_at":"2018-12-17T17:59:28Z","abstract_excerpt":"We have imaged the Sunyaev-Zel'dovich (SZ) effect signals at 140 and 270 GHz towards ten galaxy clusters with Bolocam and AzTEC/ASTE. We also used Planck data to constrain the signal at large angular scales, Herschel-SPIRE images to subtract the brightest galaxies that comprise the cosmic infrared background (CIB), Chandra imaging to map the electron temperature $T_e$ of the intra-cluster medium (ICM), and HST imaging to derive models of each galaxy cluster's mass density. The galaxy clusters gravitationally lens the background CIB, which produced an on-average reduction in brightness towards "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.06926","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1812.06926/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":"1812.06926","created_at":"2026-07-04T23:50:13.815533+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.06926v2","created_at":"2026-07-04T23:50:13.815533+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.06926","created_at":"2026-07-04T23:50:13.815533+00:00"},{"alias_kind":"pith_short_12","alias_value":"QEPW7MWOLA5E","created_at":"2026-07-04T23:50:13.815533+00:00"},{"alias_kind":"pith_short_16","alias_value":"QEPW7MWOLA5EABOH","created_at":"2026-07-04T23:50:13.815533+00:00"},{"alias_kind":"pith_short_8","alias_value":"QEPW7MWO","created_at":"2026-07-04T23:50:13.815533+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/QEPW7MWOLA5EABOHRC7ZKNQMOV","json":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV.json","graph_json":"https://pith.science/api/pith-number/QEPW7MWOLA5EABOHRC7ZKNQMOV/graph.json","events_json":"https://pith.science/api/pith-number/QEPW7MWOLA5EABOHRC7ZKNQMOV/events.json","paper":"https://pith.science/paper/QEPW7MWO"},"agent_actions":{"view_html":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV","download_json":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV.json","view_paper":"https://pith.science/paper/QEPW7MWO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.06926&json=true","fetch_graph":"https://pith.science/api/pith-number/QEPW7MWOLA5EABOHRC7ZKNQMOV/graph.json","fetch_events":"https://pith.science/api/pith-number/QEPW7MWOLA5EABOHRC7ZKNQMOV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV/action/storage_attestation","attest_author":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV/action/author_attestation","sign_citation":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV/action/citation_signature","submit_replication":"https://pith.science/pith/QEPW7MWOLA5EABOHRC7ZKNQMOV/action/replication_record"}},"created_at":"2026-07-04T23:50:13.815533+00:00","updated_at":"2026-07-04T23:50:13.815533+00:00"}