{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:EKTAWFGECGRWG233TFYAWSLR2X","short_pith_number":"pith:EKTAWFGE","schema_version":"1.0","canonical_sha256":"22a60b14c411a3636b7b99700b4971d5caf1b4c82a32a195e42eb98bca4d7136","source":{"kind":"arxiv","id":"1005.4699","version":1},"attestation_state":"computed","paper":{"title":"A high signal to noise ratio map of the Sunyaev-Zel'dovich increment at 1.1 mm wavelength in Abell 1835","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Eiichi Egami, Glenn Laurent, Hien Nguyen, Jack Sayers, James Aguirre, Jamie Bock, Jason Glenn, Philip Mauskopf, Piers Horner, Sunil Golwala","submitted_at":"2010-05-25T20:46:17Z","abstract_excerpt":"We present an analysis of an 8 arcminute diameter map of the area around the galaxy cluster Abell 1835 from jiggle map observations at a wavelength of 1.1 mm using the Bolometric Camera (Bolocam) mounted on the Caltech Submillimeter Observatory (CSO). The data is well described by a model including an extended Sunyaev-Zel'dovich (SZ) signal from the cluster gas plus emission from two bright background submm galaxies magnified by the gravitational lensing of the cluster. The best-fit values for the central Compton value for the cluster and the fluxes of the two main point sources in the field: "},"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":"1005.4699","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-05-25T20:46:17Z","cross_cats_sorted":[],"title_canon_sha256":"46860cc468faf61b2600e5ce2e622a46e2d82139ce176cadd4ba6c2c6228ee6b","abstract_canon_sha256":"bd67b4cf7c42c5efa2bc02ade653c7efa04fb201449aa2f3761bf6d300426ee0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:29:24.267540Z","signature_b64":"RfAene/LA68bclbHhueCZaB7CxgTZdrXmhHqYKxDMW2zBRkc+ECcQv3AII11jb3jiQSCXF00tQ9fOdeKXEdjAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"22a60b14c411a3636b7b99700b4971d5caf1b4c82a32a195e42eb98bca4d7136","last_reissued_at":"2026-07-04T17:29:24.267110Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:29:24.267110Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A high signal to noise ratio map of the Sunyaev-Zel'dovich increment at 1.1 mm wavelength in Abell 1835","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Eiichi Egami, Glenn Laurent, Hien Nguyen, Jack Sayers, James Aguirre, Jamie Bock, Jason Glenn, Philip Mauskopf, Piers Horner, Sunil Golwala","submitted_at":"2010-05-25T20:46:17Z","abstract_excerpt":"We present an analysis of an 8 arcminute diameter map of the area around the galaxy cluster Abell 1835 from jiggle map observations at a wavelength of 1.1 mm using the Bolometric Camera (Bolocam) mounted on the Caltech Submillimeter Observatory (CSO). The data is well described by a model including an extended Sunyaev-Zel'dovich (SZ) signal from the cluster gas plus emission from two bright background submm galaxies magnified by the gravitational lensing of the cluster. The best-fit values for the central Compton value for the cluster and the fluxes of the two main point sources in the field: "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.4699","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/1005.4699/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":"1005.4699","created_at":"2026-07-04T17:29:24.267175+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.4699v1","created_at":"2026-07-04T17:29:24.267175+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.4699","created_at":"2026-07-04T17:29:24.267175+00:00"},{"alias_kind":"pith_short_12","alias_value":"EKTAWFGECGRW","created_at":"2026-07-04T17:29:24.267175+00:00"},{"alias_kind":"pith_short_16","alias_value":"EKTAWFGECGRWG233","created_at":"2026-07-04T17:29:24.267175+00:00"},{"alias_kind":"pith_short_8","alias_value":"EKTAWFGE","created_at":"2026-07-04T17:29:24.267175+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/EKTAWFGECGRWG233TFYAWSLR2X","json":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X.json","graph_json":"https://pith.science/api/pith-number/EKTAWFGECGRWG233TFYAWSLR2X/graph.json","events_json":"https://pith.science/api/pith-number/EKTAWFGECGRWG233TFYAWSLR2X/events.json","paper":"https://pith.science/paper/EKTAWFGE"},"agent_actions":{"view_html":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X","download_json":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X.json","view_paper":"https://pith.science/paper/EKTAWFGE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.4699&json=true","fetch_graph":"https://pith.science/api/pith-number/EKTAWFGECGRWG233TFYAWSLR2X/graph.json","fetch_events":"https://pith.science/api/pith-number/EKTAWFGECGRWG233TFYAWSLR2X/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X/action/storage_attestation","attest_author":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X/action/author_attestation","sign_citation":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X/action/citation_signature","submit_replication":"https://pith.science/pith/EKTAWFGECGRWG233TFYAWSLR2X/action/replication_record"}},"created_at":"2026-07-04T17:29:24.267175+00:00","updated_at":"2026-07-04T17:29:24.267175+00:00"}