{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:GZ554VHL3D5QRZEM2W74TD6LUQ","short_pith_number":"pith:GZ554VHL","schema_version":"1.0","canonical_sha256":"367bde54ebd8fb08e48cd5bfc98fcba434a0b77b5bb30f187d73eca018fbb2f8","source":{"kind":"arxiv","id":"1410.3883","version":1},"attestation_state":"computed","paper":{"title":"Comparing Dense Galaxy Cluster Redshift Surveys with Weak Lensing Maps","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Antonaldo Diaferio, H. Jabran Zahid, Ho Seong Hwang, Kenneth J. Rines, Margaret J. Geller","submitted_at":"2014-10-14T22:32:20Z","abstract_excerpt":"We use dense redshift surveys of nine galaxy clusters at $z\\sim0.2$ to compare the galaxy distribution in each system with the projected matter distribution from weak lensing. By combining 2087 new MMT/Hectospec redshifts and the data in the literature, we construct spectroscopic samples within the region of weak-lensing maps of high (70--89%) and uniform completeness. With these dense redshift surveys, we construct galaxy number density maps using several galaxy subsamples. The shape of the main cluster concentration in the weak-lensing maps is similar to the global morphology of the number d"},"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":"1410.3883","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-10-14T22:32:20Z","cross_cats_sorted":[],"title_canon_sha256":"fbd9aec811dbca562837da4cb1804d4dce9d5ea25bbf8bbb1e344d43e637a431","abstract_canon_sha256":"177537f4eaa956cbd428cb3f9859b294eb260a70d067409e6151bdccf0e45698"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:48.350560Z","signature_b64":"SsALifms4ArF3Doj7W02HOCRZLUQAr3Xh/S8D7+lMXQFQEuX73WkDVGHMAWOlxuutfSYooppAgRM+o7b9oSiBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"367bde54ebd8fb08e48cd5bfc98fcba434a0b77b5bb30f187d73eca018fbb2f8","last_reissued_at":"2026-05-18T01:41:48.350049Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:48.350049Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Comparing Dense Galaxy Cluster Redshift Surveys with Weak Lensing Maps","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Antonaldo Diaferio, H. Jabran Zahid, Ho Seong Hwang, Kenneth J. Rines, Margaret J. Geller","submitted_at":"2014-10-14T22:32:20Z","abstract_excerpt":"We use dense redshift surveys of nine galaxy clusters at $z\\sim0.2$ to compare the galaxy distribution in each system with the projected matter distribution from weak lensing. By combining 2087 new MMT/Hectospec redshifts and the data in the literature, we construct spectroscopic samples within the region of weak-lensing maps of high (70--89%) and uniform completeness. With these dense redshift surveys, we construct galaxy number density maps using several galaxy subsamples. The shape of the main cluster concentration in the weak-lensing maps is similar to the global morphology of the number d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.3883","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":""},"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":"1410.3883","created_at":"2026-05-18T01:41:48.350143+00:00"},{"alias_kind":"arxiv_version","alias_value":"1410.3883v1","created_at":"2026-05-18T01:41:48.350143+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.3883","created_at":"2026-05-18T01:41:48.350143+00:00"},{"alias_kind":"pith_short_12","alias_value":"GZ554VHL3D5Q","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_16","alias_value":"GZ554VHL3D5QRZEM","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_8","alias_value":"GZ554VHL","created_at":"2026-05-18T12:28:30.664211+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/GZ554VHL3D5QRZEM2W74TD6LUQ","json":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ.json","graph_json":"https://pith.science/api/pith-number/GZ554VHL3D5QRZEM2W74TD6LUQ/graph.json","events_json":"https://pith.science/api/pith-number/GZ554VHL3D5QRZEM2W74TD6LUQ/events.json","paper":"https://pith.science/paper/GZ554VHL"},"agent_actions":{"view_html":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ","download_json":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ.json","view_paper":"https://pith.science/paper/GZ554VHL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1410.3883&json=true","fetch_graph":"https://pith.science/api/pith-number/GZ554VHL3D5QRZEM2W74TD6LUQ/graph.json","fetch_events":"https://pith.science/api/pith-number/GZ554VHL3D5QRZEM2W74TD6LUQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/action/storage_attestation","attest_author":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/action/author_attestation","sign_citation":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/action/citation_signature","submit_replication":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/action/replication_record"}},"created_at":"2026-05-18T01:41:48.350143+00:00","updated_at":"2026-05-18T01:41:48.350143+00:00"}