{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:7A3KR7LXQ33ZLFO4RNYIQTN7UO","short_pith_number":"pith:7A3KR7LX","schema_version":"1.0","canonical_sha256":"f836a8fd7786f79595dc8b70884dbfa3a74b04842f8e63ffb03fab50bfa3c85f","source":{"kind":"arxiv","id":"1705.03901","version":2},"attestation_state":"computed","paper":{"title":"Joint Strong and Weak Lensing Analysis of the Massive Cluster Field J0850+3604","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"2), (2) ASIAA, (3) Rutgers, (4) Arizona, (5) LLNL), Ann I. Zabludoff (4), Catie Raney (3), Charles R. Keeton (3), K. Decker French (4) ((1) NAOJ, Keiichi Umetsu (2), Kenneth C. Wong (1, S. Mark Ammons (5)","submitted_at":"2017-05-10T18:04:17Z","abstract_excerpt":"We present a combined strong and weak lensing analysis of the J085007.6+360428 (J0850) field, which was selected by its high projected concentration of luminous red galaxies and contains the massive cluster Zwicky 1953. Using Subaru/Suprime-Cam $BVR_{c}I_{c}i^{\\prime}z^{\\prime}$ imaging and MMT/Hectospec spectroscopy, we first perform a weak lensing shear analysis to constrain the mass distribution in this field, including the cluster at $z = 0.3774$ and a smaller foreground halo at $z = 0.2713$. We then add a strong lensing constraint from a multiply-imaged galaxy in the imaging data with a p"},"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":"1705.03901","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-10T18:04:17Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"845156ef4534bb995d01a6b301f2a477d5e7c031c7c220180c5da6bfd2995263","abstract_canon_sha256":"816939cb25111ea01d6038893f0ef664dc956f96e0e73762651eca2f89d1f824"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:27.273734Z","signature_b64":"V00SJSuQiAlVwduA4NFjC6U+DleUXr56n/cKKsb9E846pXVfOpcMMSSdsMfVAo/tvoqZUurtUZJRP5dvYDGeDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f836a8fd7786f79595dc8b70884dbfa3a74b04842f8e63ffb03fab50bfa3c85f","last_reissued_at":"2026-05-18T00:38:27.272979Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:27.272979Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Joint Strong and Weak Lensing Analysis of the Massive Cluster Field J0850+3604","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"2), (2) ASIAA, (3) Rutgers, (4) Arizona, (5) LLNL), Ann I. Zabludoff (4), Catie Raney (3), Charles R. Keeton (3), K. Decker French (4) ((1) NAOJ, Keiichi Umetsu (2), Kenneth C. Wong (1, S. Mark Ammons (5)","submitted_at":"2017-05-10T18:04:17Z","abstract_excerpt":"We present a combined strong and weak lensing analysis of the J085007.6+360428 (J0850) field, which was selected by its high projected concentration of luminous red galaxies and contains the massive cluster Zwicky 1953. Using Subaru/Suprime-Cam $BVR_{c}I_{c}i^{\\prime}z^{\\prime}$ imaging and MMT/Hectospec spectroscopy, we first perform a weak lensing shear analysis to constrain the mass distribution in this field, including the cluster at $z = 0.3774$ and a smaller foreground halo at $z = 0.2713$. We then add a strong lensing constraint from a multiply-imaged galaxy in the imaging data with a p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.03901","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":"1705.03901","created_at":"2026-05-18T00:38:27.273116+00:00"},{"alias_kind":"arxiv_version","alias_value":"1705.03901v2","created_at":"2026-05-18T00:38:27.273116+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.03901","created_at":"2026-05-18T00:38:27.273116+00:00"},{"alias_kind":"pith_short_12","alias_value":"7A3KR7LXQ33Z","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_16","alias_value":"7A3KR7LXQ33ZLFO4","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_8","alias_value":"7A3KR7LX","created_at":"2026-05-18T12:31:03.183658+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/7A3KR7LXQ33ZLFO4RNYIQTN7UO","json":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO.json","graph_json":"https://pith.science/api/pith-number/7A3KR7LXQ33ZLFO4RNYIQTN7UO/graph.json","events_json":"https://pith.science/api/pith-number/7A3KR7LXQ33ZLFO4RNYIQTN7UO/events.json","paper":"https://pith.science/paper/7A3KR7LX"},"agent_actions":{"view_html":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO","download_json":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO.json","view_paper":"https://pith.science/paper/7A3KR7LX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1705.03901&json=true","fetch_graph":"https://pith.science/api/pith-number/7A3KR7LXQ33ZLFO4RNYIQTN7UO/graph.json","fetch_events":"https://pith.science/api/pith-number/7A3KR7LXQ33ZLFO4RNYIQTN7UO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO/action/storage_attestation","attest_author":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO/action/author_attestation","sign_citation":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO/action/citation_signature","submit_replication":"https://pith.science/pith/7A3KR7LXQ33ZLFO4RNYIQTN7UO/action/replication_record"}},"created_at":"2026-05-18T00:38:27.273116+00:00","updated_at":"2026-05-18T00:38:27.273116+00:00"}