{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:T2JR5IX6FYJEFBS4W62LSTV2JZ","short_pith_number":"pith:T2JR5IX6","canonical_record":{"source":{"id":"1006.5121","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-26T08:32:53Z","cross_cats_sorted":[],"title_canon_sha256":"89a1f59458b0b523a51c43f2f016dc4dee1d43eda7e16a02e238c1bf6d44e242","abstract_canon_sha256":"0aeedb7e0f0b7e0acdb85434a8a19af6f96cffaba8387783515d160babb76061"},"schema_version":"1.0"},"canonical_sha256":"9e931ea2fe2e1242865cb7b4b94eba4e54428327ebb6445e8c80f2b31f0855de","source":{"kind":"arxiv","id":"1006.5121","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.5121","created_at":"2026-05-18T02:06:35Z"},{"alias_kind":"arxiv_version","alias_value":"1006.5121v1","created_at":"2026-05-18T02:06:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.5121","created_at":"2026-05-18T02:06:35Z"},{"alias_kind":"pith_short_12","alias_value":"T2JR5IX6FYJE","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_16","alias_value":"T2JR5IX6FYJEFBS4","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_8","alias_value":"T2JR5IX6","created_at":"2026-05-18T12:26:13Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:T2JR5IX6FYJEFBS4W62LSTV2JZ","target":"record","payload":{"canonical_record":{"source":{"id":"1006.5121","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-26T08:32:53Z","cross_cats_sorted":[],"title_canon_sha256":"89a1f59458b0b523a51c43f2f016dc4dee1d43eda7e16a02e238c1bf6d44e242","abstract_canon_sha256":"0aeedb7e0f0b7e0acdb85434a8a19af6f96cffaba8387783515d160babb76061"},"schema_version":"1.0"},"canonical_sha256":"9e931ea2fe2e1242865cb7b4b94eba4e54428327ebb6445e8c80f2b31f0855de","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:35.290901Z","signature_b64":"TjUXf24k9uWuEd6yxVeFpuuOEqcP0J+fxIb+DYVCqzWE3JYZ8Nm7sX2GD2i9ZNjVTv/NOCo0mP3cTdaK5qHgAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e931ea2fe2e1242865cb7b4b94eba4e54428327ebb6445e8c80f2b31f0855de","last_reissued_at":"2026-05-18T02:06:35.290194Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:35.290194Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1006.5121","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:06:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"mp6GPkg8mEr/QMnBW7K0ZvPTb526Sp43GfmnLjsnxlig1N0D2VLwGu+Jeb7R34Q1a7feUyymDIuvGBEK2yCyBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-05T05:40:46.372530Z"},"content_sha256":"193d3926db99aa7422d0ca9269e5c769478390ca38f47d4e436da99b505dcc97","schema_version":"1.0","event_id":"sha256:193d3926db99aa7422d0ca9269e5c769478390ca38f47d4e436da99b505dcc97"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:T2JR5IX6FYJEFBS4W62LSTV2JZ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Noisy weak-lensing convergence peak statistics near clusters of galaxies and beyond","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Huanyuan Shan, Jiayi Liu, Zuhui Fan","submitted_at":"2010-06-26T08:32:53Z","abstract_excerpt":"Taking into account noise from intrinsic ellipticities of source galaxies, in this paper, we study the peak statistics in weak-lensing convergence maps around clusters of galaxies and beyond. We emphasize how the noise peak statistics is affected by the density distribution of nearby clusters, and also how cluster-peak signals are changed by the existence of noise. These are the important aspects to be understood thoroughly in weak-lensing analyses for individual clusters as well as in cosmological applications of weak-lensing cluster statistics. We adopt Gaussian smoothing with the smoothing "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.5121","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:06:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7jys6/MTXrdZorozhjwVG7/IygYwuMhOos0vlmDFpCP4ogEZLN0fCCGhkbmahUHwzU3gaUTf34YgJ03dxxD8Aw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-07-05T05:40:46.372877Z"},"content_sha256":"34c9d56c623425edaec6f2bc68d16a62a85ddf19fe9de72317472ccf1d5f0a83","schema_version":"1.0","event_id":"sha256:34c9d56c623425edaec6f2bc68d16a62a85ddf19fe9de72317472ccf1d5f0a83"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/T2JR5IX6FYJEFBS4W62LSTV2JZ/bundle.json","state_url":"https://pith.science/pith/T2JR5IX6FYJEFBS4W62LSTV2JZ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/T2JR5IX6FYJEFBS4W62LSTV2JZ/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":"2026-07-05T05:40:46Z","links":{"resolver":"https://pith.science/pith/T2JR5IX6FYJEFBS4W62LSTV2JZ","bundle":"https://pith.science/pith/T2JR5IX6FYJEFBS4W62LSTV2JZ/bundle.json","state":"https://pith.science/pith/T2JR5IX6FYJEFBS4W62LSTV2JZ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/T2JR5IX6FYJEFBS4W62LSTV2JZ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:T2JR5IX6FYJEFBS4W62LSTV2JZ","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":"0aeedb7e0f0b7e0acdb85434a8a19af6f96cffaba8387783515d160babb76061","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-26T08:32:53Z","title_canon_sha256":"89a1f59458b0b523a51c43f2f016dc4dee1d43eda7e16a02e238c1bf6d44e242"},"schema_version":"1.0","source":{"id":"1006.5121","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.5121","created_at":"2026-05-18T02:06:35Z"},{"alias_kind":"arxiv_version","alias_value":"1006.5121v1","created_at":"2026-05-18T02:06:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.5121","created_at":"2026-05-18T02:06:35Z"},{"alias_kind":"pith_short_12","alias_value":"T2JR5IX6FYJE","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_16","alias_value":"T2JR5IX6FYJEFBS4","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_8","alias_value":"T2JR5IX6","created_at":"2026-05-18T12:26:13Z"}],"graph_snapshots":[{"event_id":"sha256:34c9d56c623425edaec6f2bc68d16a62a85ddf19fe9de72317472ccf1d5f0a83","target":"graph","created_at":"2026-05-18T02:06:35Z","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":"Taking into account noise from intrinsic ellipticities of source galaxies, in this paper, we study the peak statistics in weak-lensing convergence maps around clusters of galaxies and beyond. We emphasize how the noise peak statistics is affected by the density distribution of nearby clusters, and also how cluster-peak signals are changed by the existence of noise. These are the important aspects to be understood thoroughly in weak-lensing analyses for individual clusters as well as in cosmological applications of weak-lensing cluster statistics. We adopt Gaussian smoothing with the smoothing ","authors_text":"Huanyuan Shan, Jiayi Liu, Zuhui Fan","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-26T08:32:53Z","title":"Noisy weak-lensing convergence peak statistics near clusters of galaxies and beyond"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.5121","kind":"arxiv","version":1},"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":"sha256:193d3926db99aa7422d0ca9269e5c769478390ca38f47d4e436da99b505dcc97","target":"record","created_at":"2026-05-18T02:06:35Z","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":"0aeedb7e0f0b7e0acdb85434a8a19af6f96cffaba8387783515d160babb76061","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-26T08:32:53Z","title_canon_sha256":"89a1f59458b0b523a51c43f2f016dc4dee1d43eda7e16a02e238c1bf6d44e242"},"schema_version":"1.0","source":{"id":"1006.5121","kind":"arxiv","version":1}},"canonical_sha256":"9e931ea2fe2e1242865cb7b4b94eba4e54428327ebb6445e8c80f2b31f0855de","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"9e931ea2fe2e1242865cb7b4b94eba4e54428327ebb6445e8c80f2b31f0855de","first_computed_at":"2026-05-18T02:06:35.290194Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:06:35.290194Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"TjUXf24k9uWuEd6yxVeFpuuOEqcP0J+fxIb+DYVCqzWE3JYZ8Nm7sX2GD2i9ZNjVTv/NOCo0mP3cTdaK5qHgAg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:06:35.290901Z","signed_message":"canonical_sha256_bytes"},"source_id":"1006.5121","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:193d3926db99aa7422d0ca9269e5c769478390ca38f47d4e436da99b505dcc97","sha256:34c9d56c623425edaec6f2bc68d16a62a85ddf19fe9de72317472ccf1d5f0a83"],"state_sha256":"8a727edd561b7cfcba0ca978fbae25bee8d691187559bd877d20aca04955852c"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"VSuRc9/uLUV2fBrAPRvVd+L8ssoA6x5s25n5mB0Rku95qxDPblYpQ5oB0cMdXMcZxiJLhIDP3OuW2/mV3W0VBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-07-05T05:40:46.374898Z","bundle_sha256":"d2becd2598b2dacd72872d753b7535f50613bf7ba00d969af892232f8e68f845"}}