{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:3N43UEOXIYWEJU2ZX456DLXRBZ","short_pith_number":"pith:3N43UEOX","canonical_record":{"source":{"id":"1106.2046","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-06-10T13:16:21Z","cross_cats_sorted":[],"title_canon_sha256":"5d27d3355c264270b5e44797543f74766c70c3223c9428e9d2b5f1b3c180d07e","abstract_canon_sha256":"22e25ea1a39ce4e3f2c48c51e42360a38f7b4579a77d95a700f6e07019b029ed"},"schema_version":"1.0"},"canonical_sha256":"db79ba11d7462c44d359bf3be1aef10e5b35ba67ffbb1a47d65ed877d96600aa","source":{"kind":"arxiv","id":"1106.2046","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1106.2046","created_at":"2026-05-18T03:55:56Z"},{"alias_kind":"arxiv_version","alias_value":"1106.2046v3","created_at":"2026-05-18T03:55:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.2046","created_at":"2026-05-18T03:55:56Z"},{"alias_kind":"pith_short_12","alias_value":"3N43UEOXIYWE","created_at":"2026-05-18T12:26:18Z"},{"alias_kind":"pith_short_16","alias_value":"3N43UEOXIYWEJU2Z","created_at":"2026-05-18T12:26:18Z"},{"alias_kind":"pith_short_8","alias_value":"3N43UEOX","created_at":"2026-05-18T12:26:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:3N43UEOXIYWEJU2ZX456DLXRBZ","target":"record","payload":{"canonical_record":{"source":{"id":"1106.2046","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-06-10T13:16:21Z","cross_cats_sorted":[],"title_canon_sha256":"5d27d3355c264270b5e44797543f74766c70c3223c9428e9d2b5f1b3c180d07e","abstract_canon_sha256":"22e25ea1a39ce4e3f2c48c51e42360a38f7b4579a77d95a700f6e07019b029ed"},"schema_version":"1.0"},"canonical_sha256":"db79ba11d7462c44d359bf3be1aef10e5b35ba67ffbb1a47d65ed877d96600aa","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:55:56.163576Z","signature_b64":"mJCRdxgLbbbLQKbsLh30slyrfYUVYk4ap1klQsBThS3tfrlnU+21OfosrvlmuY9lg6uGfn0UH5S4Vr3qz8bNCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"db79ba11d7462c44d359bf3be1aef10e5b35ba67ffbb1a47d65ed877d96600aa","last_reissued_at":"2026-05-18T03:55:56.162798Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:55:56.162798Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1106.2046","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:55:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"eR9PjAFBB4UZuGl6w1Cr/CUrvhRkIf+vaJKMK/rkeuYNjbmw7rvCjNwbzwYx4S0erMKmLiwEO5HvzqJ0RzYIBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-24T10:14:22.461894Z"},"content_sha256":"8f8057ab66313db8d6f52d729bd88c647900c1e4f3c5e2c878859f20d7d82ec0","schema_version":"1.0","event_id":"sha256:8f8057ab66313db8d6f52d729bd88c647900c1e4f3c5e2c878859f20d7d82ec0"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:3N43UEOXIYWEJU2ZX456DLXRBZ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"1), 2) ((1) Institute of Astronomy, (2) Kavli Institute for Cosmology, Cambridge, Cambridge), Ian G. McCarthy (2, Lindsay J. King (1, Yannick M. Bah\\'e (1)","submitted_at":"2011-06-10T13:16:21Z","abstract_excerpt":"(Abridged) We quantify the bias and scatter in galaxy cluster masses and concentrations derived from an idealised mock weak gravitational lensing (WL) survey, and their effect on the cluster mass-concentration relation. For this, we simulate WL distortions on a population of background galaxies due to a large (~3000) sample of galaxy cluster haloes extracted from the Millennium Simulation at z~0.2. This study takes into account the influence of shape noise, cluster substructure and asphericity as well as correlated large-scale structure, but not uncorrelated large-scale structure along the lin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.2046","kind":"arxiv","version":3},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:55:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"+gcbvcfowrAr5izPHsaoq7bAc3jnuvOE9R3G6eRMvmCNnPVU6IuJithz0N3c4SE9yC2k7epX2Max1kyf90qECg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-24T10:14:22.462364Z"},"content_sha256":"2268a548d283012e358ce26d489e404020c1f3996c7e410aaaaf8a7db7788a7e","schema_version":"1.0","event_id":"sha256:2268a548d283012e358ce26d489e404020c1f3996c7e410aaaaf8a7db7788a7e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/3N43UEOXIYWEJU2ZX456DLXRBZ/bundle.json","state_url":"https://pith.science/pith/3N43UEOXIYWEJU2ZX456DLXRBZ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/3N43UEOXIYWEJU2ZX456DLXRBZ/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-24T10:14:22Z","links":{"resolver":"https://pith.science/pith/3N43UEOXIYWEJU2ZX456DLXRBZ","bundle":"https://pith.science/pith/3N43UEOXIYWEJU2ZX456DLXRBZ/bundle.json","state":"https://pith.science/pith/3N43UEOXIYWEJU2ZX456DLXRBZ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/3N43UEOXIYWEJU2ZX456DLXRBZ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:3N43UEOXIYWEJU2ZX456DLXRBZ","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"22e25ea1a39ce4e3f2c48c51e42360a38f7b4579a77d95a700f6e07019b029ed","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-06-10T13:16:21Z","title_canon_sha256":"5d27d3355c264270b5e44797543f74766c70c3223c9428e9d2b5f1b3c180d07e"},"schema_version":"1.0","source":{"id":"1106.2046","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1106.2046","created_at":"2026-05-18T03:55:56Z"},{"alias_kind":"arxiv_version","alias_value":"1106.2046v3","created_at":"2026-05-18T03:55:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.2046","created_at":"2026-05-18T03:55:56Z"},{"alias_kind":"pith_short_12","alias_value":"3N43UEOXIYWE","created_at":"2026-05-18T12:26:18Z"},{"alias_kind":"pith_short_16","alias_value":"3N43UEOXIYWEJU2Z","created_at":"2026-05-18T12:26:18Z"},{"alias_kind":"pith_short_8","alias_value":"3N43UEOX","created_at":"2026-05-18T12:26:18Z"}],"graph_snapshots":[{"event_id":"sha256:2268a548d283012e358ce26d489e404020c1f3996c7e410aaaaf8a7db7788a7e","target":"graph","created_at":"2026-05-18T03:55:56Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"(Abridged) We quantify the bias and scatter in galaxy cluster masses and concentrations derived from an idealised mock weak gravitational lensing (WL) survey, and their effect on the cluster mass-concentration relation. For this, we simulate WL distortions on a population of background galaxies due to a large (~3000) sample of galaxy cluster haloes extracted from the Millennium Simulation at z~0.2. This study takes into account the influence of shape noise, cluster substructure and asphericity as well as correlated large-scale structure, but not uncorrelated large-scale structure along the lin","authors_text":"1), 2) ((1) Institute of Astronomy, (2) Kavli Institute for Cosmology, Cambridge, Cambridge), Ian G. McCarthy (2, Lindsay J. King (1, Yannick M. Bah\\'e (1)","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-06-10T13:16:21Z","title":"Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.2046","kind":"arxiv","version":3},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:8f8057ab66313db8d6f52d729bd88c647900c1e4f3c5e2c878859f20d7d82ec0","target":"record","created_at":"2026-05-18T03:55:56Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"22e25ea1a39ce4e3f2c48c51e42360a38f7b4579a77d95a700f6e07019b029ed","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-06-10T13:16:21Z","title_canon_sha256":"5d27d3355c264270b5e44797543f74766c70c3223c9428e9d2b5f1b3c180d07e"},"schema_version":"1.0","source":{"id":"1106.2046","kind":"arxiv","version":3}},"canonical_sha256":"db79ba11d7462c44d359bf3be1aef10e5b35ba67ffbb1a47d65ed877d96600aa","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"db79ba11d7462c44d359bf3be1aef10e5b35ba67ffbb1a47d65ed877d96600aa","first_computed_at":"2026-05-18T03:55:56.162798Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:55:56.162798Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"mJCRdxgLbbbLQKbsLh30slyrfYUVYk4ap1klQsBThS3tfrlnU+21OfosrvlmuY9lg6uGfn0UH5S4Vr3qz8bNCg==","signature_status":"signed_v1","signed_at":"2026-05-18T03:55:56.163576Z","signed_message":"canonical_sha256_bytes"},"source_id":"1106.2046","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8f8057ab66313db8d6f52d729bd88c647900c1e4f3c5e2c878859f20d7d82ec0","sha256:2268a548d283012e358ce26d489e404020c1f3996c7e410aaaaf8a7db7788a7e"],"state_sha256":"73d91d1801bcb01f8d1d9f96f34f07658b7823a46ca4d2d0e75cfa51873f6c45"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mUldpS3nKHeDIE0URMX2gs5nJnxXzeRtxk8ziRyRJOkqe7QGbB8J5eQ7dlIndcsoWGF8V3kPhxDguucoRv3FBg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-24T10:14:22.466132Z","bundle_sha256":"6d9f86f4ed210284ccf532a05101fa6a966c3513cdf0e4ccb51b7f219fc83d65"}}