{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:LVNDQFBRDWHDEBIPKF6QMHUXK4","short_pith_number":"pith:LVNDQFBR","schema_version":"1.0","canonical_sha256":"5d5a3814311d8e32050f517d061e97572b9f813e28e98afeae6ed1c048cf3df0","source":{"kind":"arxiv","id":"2312.11789","version":1},"attestation_state":"computed","paper":{"title":"Forecasting the constraints on optical selection bias and projection effects of galaxy cluster lensing with multiwavelength data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Alexie Leauthaud, Andr\\'es N. Salcedo, Chun-Hao To, Conghao Zhou, David H. Weinberg, Eduardo Rozo, Hao-Yi Wu, Matteo Costanzi, Matthew Kwiecien, Sebastian Bocquet, Sebastian Grandis, Tamas Varga, Tesla Jeltema, Tianyu Zhang, Tomomi Sunayama","submitted_at":"2023-12-19T01:54:48Z","abstract_excerpt":"Galaxy clusters identified with optical imaging tend to suffer from projection effects, which impact richness (the number of member galaxies in a cluster) and lensing coherently. Physically unassociated galaxies can be mistaken as cluster members due to the significant uncertainties in their line-of-sight distances, thereby changing the observed cluster richness; at the same time, projection effects alter the weak gravitational lensing signals of clusters, leading to a correlated scatter between richness and lensing at a given halo mass. As a result, the lensing signals for optically selected "},"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":"2312.11789","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-12-19T01:54:48Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"ce8e7c2a2d738370612356dbf6909587adaff782da0b61d45dd96a81ae8e763c","abstract_canon_sha256":"f7f3dbca710278f36e5f2293f7faf9ac9708c18e9f8ec28961bbdc2d2234da1c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:25:54.271145Z","signature_b64":"B6kiAJhVrIqxsCADlNV3D9VFNJr9Nz55JMvLtmffsXIAMi4cltYH8qv7tLc0Ee+dbl7GVb65zQJOcYfI1w50AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5d5a3814311d8e32050f517d061e97572b9f813e28e98afeae6ed1c048cf3df0","last_reissued_at":"2026-07-05T07:25:54.270701Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:25:54.270701Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Forecasting the constraints on optical selection bias and projection effects of galaxy cluster lensing with multiwavelength data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Alexie Leauthaud, Andr\\'es N. Salcedo, Chun-Hao To, Conghao Zhou, David H. Weinberg, Eduardo Rozo, Hao-Yi Wu, Matteo Costanzi, Matthew Kwiecien, Sebastian Bocquet, Sebastian Grandis, Tamas Varga, Tesla Jeltema, Tianyu Zhang, Tomomi Sunayama","submitted_at":"2023-12-19T01:54:48Z","abstract_excerpt":"Galaxy clusters identified with optical imaging tend to suffer from projection effects, which impact richness (the number of member galaxies in a cluster) and lensing coherently. Physically unassociated galaxies can be mistaken as cluster members due to the significant uncertainties in their line-of-sight distances, thereby changing the observed cluster richness; at the same time, projection effects alter the weak gravitational lensing signals of clusters, leading to a correlated scatter between richness and lensing at a given halo mass. As a result, the lensing signals for optically selected "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.11789","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/2312.11789/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":"2312.11789","created_at":"2026-07-05T07:25:54.270757+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.11789v1","created_at":"2026-07-05T07:25:54.270757+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.11789","created_at":"2026-07-05T07:25:54.270757+00:00"},{"alias_kind":"pith_short_12","alias_value":"LVNDQFBRDWHD","created_at":"2026-07-05T07:25:54.270757+00:00"},{"alias_kind":"pith_short_16","alias_value":"LVNDQFBRDWHDEBIP","created_at":"2026-07-05T07:25:54.270757+00:00"},{"alias_kind":"pith_short_8","alias_value":"LVNDQFBR","created_at":"2026-07-05T07:25:54.270757+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2510.00753","citing_title":"Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters","ref_index":85,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4","json":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4.json","graph_json":"https://pith.science/api/pith-number/LVNDQFBRDWHDEBIPKF6QMHUXK4/graph.json","events_json":"https://pith.science/api/pith-number/LVNDQFBRDWHDEBIPKF6QMHUXK4/events.json","paper":"https://pith.science/paper/LVNDQFBR"},"agent_actions":{"view_html":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4","download_json":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4.json","view_paper":"https://pith.science/paper/LVNDQFBR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.11789&json=true","fetch_graph":"https://pith.science/api/pith-number/LVNDQFBRDWHDEBIPKF6QMHUXK4/graph.json","fetch_events":"https://pith.science/api/pith-number/LVNDQFBRDWHDEBIPKF6QMHUXK4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4/action/storage_attestation","attest_author":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4/action/author_attestation","sign_citation":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4/action/citation_signature","submit_replication":"https://pith.science/pith/LVNDQFBRDWHDEBIPKF6QMHUXK4/action/replication_record"}},"created_at":"2026-07-05T07:25:54.270757+00:00","updated_at":"2026-07-05T07:25:54.270757+00:00"}