{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:QAELGMCS4TZX57QW5RGNEWIFPT","short_pith_number":"pith:QAELGMCS","schema_version":"1.0","canonical_sha256":"8008b33052e4f37efe16ec4cd259057cfda87b31f5d680b21337a4244859dcc3","source":{"kind":"arxiv","id":"1605.03541","version":2},"attestation_state":"computed","paper":{"title":"A Comparison and Joint Analysis of Sunyaev-Zel'dovich Effect Measurements from Planck and Bolocam for a set of 47 Massive Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam B. Mantz, Ben Wolman, Elena Pierpaoli, Gregory Pailet, Jack Sayers, Julian Merten, Michael Naka, Sandor M. Molnar, Seth R. Siegel, Sunil R. Golwala","submitted_at":"2016-05-11T18:40:56Z","abstract_excerpt":"We measure the SZ signal toward a set of 47 clusters with a median mass of $9.5 \\times 10^{14}$ M$_{\\odot}$ and a median redshift of 0.40 using data from Planck and the ground-based Bolocam receiver. When Planck XMM-like masses are used to set the scale radius $\\theta_{\\textrm{s}}$, we find consistency between the integrated SZ signal, $Y_{\\textrm{5R500}}$, derived from Bolocam and Planck based on gNFW model fits using A10 shape parameters, with an average ratio of $1.069 \\pm 0.030$ (allowing for the $\\simeq 5$% Bolocam flux calibration uncertainty). We also perform a joint fit to the Bolocam "},"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":"1605.03541","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-05-11T18:40:56Z","cross_cats_sorted":[],"title_canon_sha256":"3ac08974dec25152efd558d1edb04bb0e4c73188d0ba21a2c6964be7cf209dbf","abstract_canon_sha256":"1bf728506255049f84818d667955f3c400fb37d1ed96a4384ddb9bfa96fbc20a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:57:12.664506Z","signature_b64":"79Q+ySTZU98906+gDsgmqys82UA3P6WBwFMtJyeRyFvc8ciunLzKAVJFugeYNUkMF/LCcAX1lYSFS4bg1wRqCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8008b33052e4f37efe16ec4cd259057cfda87b31f5d680b21337a4244859dcc3","last_reissued_at":"2026-05-18T00:57:12.663932Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:57:12.663932Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Comparison and Joint Analysis of Sunyaev-Zel'dovich Effect Measurements from Planck and Bolocam for a set of 47 Massive Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Adam B. Mantz, Ben Wolman, Elena Pierpaoli, Gregory Pailet, Jack Sayers, Julian Merten, Michael Naka, Sandor M. Molnar, Seth R. Siegel, Sunil R. Golwala","submitted_at":"2016-05-11T18:40:56Z","abstract_excerpt":"We measure the SZ signal toward a set of 47 clusters with a median mass of $9.5 \\times 10^{14}$ M$_{\\odot}$ and a median redshift of 0.40 using data from Planck and the ground-based Bolocam receiver. When Planck XMM-like masses are used to set the scale radius $\\theta_{\\textrm{s}}$, we find consistency between the integrated SZ signal, $Y_{\\textrm{5R500}}$, derived from Bolocam and Planck based on gNFW model fits using A10 shape parameters, with an average ratio of $1.069 \\pm 0.030$ (allowing for the $\\simeq 5$% Bolocam flux calibration uncertainty). We also perform a joint fit to the Bolocam "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.03541","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":"1605.03541","created_at":"2026-05-18T00:57:12.664015+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.03541v2","created_at":"2026-05-18T00:57:12.664015+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.03541","created_at":"2026-05-18T00:57:12.664015+00:00"},{"alias_kind":"pith_short_12","alias_value":"QAELGMCS4TZX","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_16","alias_value":"QAELGMCS4TZX57QW","created_at":"2026-05-18T12:30:39.010887+00:00"},{"alias_kind":"pith_short_8","alias_value":"QAELGMCS","created_at":"2026-05-18T12:30:39.010887+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/QAELGMCS4TZX57QW5RGNEWIFPT","json":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT.json","graph_json":"https://pith.science/api/pith-number/QAELGMCS4TZX57QW5RGNEWIFPT/graph.json","events_json":"https://pith.science/api/pith-number/QAELGMCS4TZX57QW5RGNEWIFPT/events.json","paper":"https://pith.science/paper/QAELGMCS"},"agent_actions":{"view_html":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT","download_json":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT.json","view_paper":"https://pith.science/paper/QAELGMCS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.03541&json=true","fetch_graph":"https://pith.science/api/pith-number/QAELGMCS4TZX57QW5RGNEWIFPT/graph.json","fetch_events":"https://pith.science/api/pith-number/QAELGMCS4TZX57QW5RGNEWIFPT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT/action/storage_attestation","attest_author":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT/action/author_attestation","sign_citation":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT/action/citation_signature","submit_replication":"https://pith.science/pith/QAELGMCS4TZX57QW5RGNEWIFPT/action/replication_record"}},"created_at":"2026-05-18T00:57:12.664015+00:00","updated_at":"2026-05-18T00:57:12.664015+00:00"}