{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FRGMO4JVP47HLSQ7D7FF2DBTZS","short_pith_number":"pith:FRGMO4JV","schema_version":"1.0","canonical_sha256":"2c4cc771357f3e75ca1f1fca5d0c33cc8ca1b1c1f5d84cf26f8f6b944b6025d8","source":{"kind":"arxiv","id":"1407.6001","version":2},"attestation_state":"computed","paper":{"title":"Optical Confirmation and Redshift Estimation of the Planck Cluster Candidates overlapping the Pan-STARRS Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. Hoyle, C. Hennig, C. Waters, C. W. Stubbs, J. J. Mohr, J. Koppenhoefer, J. Liu, J. L. Tonry, J. S. Morgan, K. C. Chambers, K. Paech, N. Kaiser, N. Metcalfe, P. A. Price, P. W. Draper, R. J. Wainscoat, S. Cole, S. Desai, W. S. Burgett","submitted_at":"2014-07-22T20:00:12Z","abstract_excerpt":"We report results of a study of Planck Sunyaev-Zel'dovich effect (SZE) selected galaxy cluster candidates using the Panoramic Survey Telescope & Rapid Response System (Pan-STARRS) imaging data. We first examine 150 Planck confirmed galaxy clusters with spectroscopic redshifts to test our algorithm for identifying optical counterparts and measuring their redshifts; our redshifts have a typical accuracy of $\\sigma_{z/(1+z)} \\sim 0.022$ for this sample. Using 60 random sky locations, we estimate that our chance of contamination through a random superposition is ~ 3 per cent. We then examine an ad"},"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":"1407.6001","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-07-22T20:00:12Z","cross_cats_sorted":[],"title_canon_sha256":"8463e4eaf2a082a21e6e31aac2f8742fa2e9b80ae2756df7c04cbfdeca705136","abstract_canon_sha256":"c21ee77794c9e86fe4b5e18c61ab8177412d85c214eb8bd3524fc0a8859cb967"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:59:58.532963Z","signature_b64":"qtuxxqb1Dp7PeZlU3OWcLPCXnjtyv/UNOPbMDDvXP7BEJpfgJfe4Ky56LxzqQD8kdZXfZHd+A3wEghvWLfQRAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2c4cc771357f3e75ca1f1fca5d0c33cc8ca1b1c1f5d84cf26f8f6b944b6025d8","last_reissued_at":"2026-05-18T01:59:58.532457Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:59:58.532457Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Optical Confirmation and Redshift Estimation of the Planck Cluster Candidates overlapping the Pan-STARRS Survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. Hoyle, C. Hennig, C. Waters, C. W. Stubbs, J. J. Mohr, J. Koppenhoefer, J. Liu, J. L. Tonry, J. S. Morgan, K. C. Chambers, K. Paech, N. Kaiser, N. Metcalfe, P. A. Price, P. W. Draper, R. J. Wainscoat, S. Cole, S. Desai, W. S. Burgett","submitted_at":"2014-07-22T20:00:12Z","abstract_excerpt":"We report results of a study of Planck Sunyaev-Zel'dovich effect (SZE) selected galaxy cluster candidates using the Panoramic Survey Telescope & Rapid Response System (Pan-STARRS) imaging data. We first examine 150 Planck confirmed galaxy clusters with spectroscopic redshifts to test our algorithm for identifying optical counterparts and measuring their redshifts; our redshifts have a typical accuracy of $\\sigma_{z/(1+z)} \\sim 0.022$ for this sample. Using 60 random sky locations, we estimate that our chance of contamination through a random superposition is ~ 3 per cent. We then examine an ad"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.6001","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":"1407.6001","created_at":"2026-05-18T01:59:58.532543+00:00"},{"alias_kind":"arxiv_version","alias_value":"1407.6001v2","created_at":"2026-05-18T01:59:58.532543+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.6001","created_at":"2026-05-18T01:59:58.532543+00:00"},{"alias_kind":"pith_short_12","alias_value":"FRGMO4JVP47H","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FRGMO4JVP47HLSQ7","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FRGMO4JV","created_at":"2026-05-18T12:28:28.263976+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/FRGMO4JVP47HLSQ7D7FF2DBTZS","json":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS.json","graph_json":"https://pith.science/api/pith-number/FRGMO4JVP47HLSQ7D7FF2DBTZS/graph.json","events_json":"https://pith.science/api/pith-number/FRGMO4JVP47HLSQ7D7FF2DBTZS/events.json","paper":"https://pith.science/paper/FRGMO4JV"},"agent_actions":{"view_html":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS","download_json":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS.json","view_paper":"https://pith.science/paper/FRGMO4JV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1407.6001&json=true","fetch_graph":"https://pith.science/api/pith-number/FRGMO4JVP47HLSQ7D7FF2DBTZS/graph.json","fetch_events":"https://pith.science/api/pith-number/FRGMO4JVP47HLSQ7D7FF2DBTZS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS/action/storage_attestation","attest_author":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS/action/author_attestation","sign_citation":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS/action/citation_signature","submit_replication":"https://pith.science/pith/FRGMO4JVP47HLSQ7D7FF2DBTZS/action/replication_record"}},"created_at":"2026-05-18T01:59:58.532543+00:00","updated_at":"2026-05-18T01:59:58.532543+00:00"}