{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:GZ554VHL3D5QRZEM2W74TD6LUQ","short_pith_number":"pith:GZ554VHL","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"},"canonical_sha256":"367bde54ebd8fb08e48cd5bfc98fcba434a0b77b5bb30f187d73eca018fbb2f8","source":{"kind":"arxiv","id":"1410.3883","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1410.3883","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"arxiv_version","alias_value":"1410.3883v1","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.3883","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"pith_short_12","alias_value":"GZ554VHL3D5Q","created_at":"2026-05-18T12:28:30Z"},{"alias_kind":"pith_short_16","alias_value":"GZ554VHL3D5QRZEM","created_at":"2026-05-18T12:28:30Z"},{"alias_kind":"pith_short_8","alias_value":"GZ554VHL","created_at":"2026-05-18T12:28:30Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:GZ554VHL3D5QRZEM2W74TD6LUQ","target":"record","payload":{"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"},"canonical_sha256":"367bde54ebd8fb08e48cd5bfc98fcba434a0b77b5bb30f187d73eca018fbb2f8","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"},"source_kind":"arxiv","source_id":"1410.3883","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":"2026-05-18T01:41:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"JL8ymPzO0DkQCLYolts8/jiuIKCUY5VLbSNk3P0qB5w85bp/dq3BxAi2gsHA3ryzAKFjWlKc23POOTGb+wtCBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T15:25:07.177370Z"},"content_sha256":"08cf86d720cb89baa2aa95aa889256035fb4c08d1a16bc6c3f28eebbdb97285e","schema_version":"1.0","event_id":"sha256:08cf86d720cb89baa2aa95aa889256035fb4c08d1a16bc6c3f28eebbdb97285e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:GZ554VHL3D5QRZEM2W74TD6LUQ","target":"graph","payload":{"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:41:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"6E+rizxFt0U21MgDe0E+d7k4Pr7mZqMV1zAGESt/e3Sg/+mrHqsUj7VdIkmitKZpfFCVUvIMXY8Bws5+TGI/Bg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T15:25:07.177721Z"},"content_sha256":"c149aee03b98d4c8622c0185a414422ba133edeab5b69d4291292689ae712457","schema_version":"1.0","event_id":"sha256:c149aee03b98d4c8622c0185a414422ba133edeab5b69d4291292689ae712457"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/bundle.json","state_url":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/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":"2026-06-04T15:25:07Z","links":{"resolver":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ","bundle":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/bundle.json","state":"https://pith.science/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GZ554VHL3D5QRZEM2W74TD6LUQ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:GZ554VHL3D5QRZEM2W74TD6LUQ","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":"177537f4eaa956cbd428cb3f9859b294eb260a70d067409e6151bdccf0e45698","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-10-14T22:32:20Z","title_canon_sha256":"fbd9aec811dbca562837da4cb1804d4dce9d5ea25bbf8bbb1e344d43e637a431"},"schema_version":"1.0","source":{"id":"1410.3883","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1410.3883","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"arxiv_version","alias_value":"1410.3883v1","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1410.3883","created_at":"2026-05-18T01:41:48Z"},{"alias_kind":"pith_short_12","alias_value":"GZ554VHL3D5Q","created_at":"2026-05-18T12:28:30Z"},{"alias_kind":"pith_short_16","alias_value":"GZ554VHL3D5QRZEM","created_at":"2026-05-18T12:28:30Z"},{"alias_kind":"pith_short_8","alias_value":"GZ554VHL","created_at":"2026-05-18T12:28:30Z"}],"graph_snapshots":[{"event_id":"sha256:c149aee03b98d4c8622c0185a414422ba133edeab5b69d4291292689ae712457","target":"graph","created_at":"2026-05-18T01:41:48Z","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":"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","authors_text":"Antonaldo Diaferio, H. Jabran Zahid, Ho Seong Hwang, Kenneth J. Rines, Margaret J. Geller","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-10-14T22:32:20Z","title":"Comparing Dense Galaxy Cluster Redshift Surveys with Weak Lensing Maps"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.3883","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":"sha256:08cf86d720cb89baa2aa95aa889256035fb4c08d1a16bc6c3f28eebbdb97285e","target":"record","created_at":"2026-05-18T01:41:48Z","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":"177537f4eaa956cbd428cb3f9859b294eb260a70d067409e6151bdccf0e45698","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2014-10-14T22:32:20Z","title_canon_sha256":"fbd9aec811dbca562837da4cb1804d4dce9d5ea25bbf8bbb1e344d43e637a431"},"schema_version":"1.0","source":{"id":"1410.3883","kind":"arxiv","version":1}},"canonical_sha256":"367bde54ebd8fb08e48cd5bfc98fcba434a0b77b5bb30f187d73eca018fbb2f8","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"367bde54ebd8fb08e48cd5bfc98fcba434a0b77b5bb30f187d73eca018fbb2f8","first_computed_at":"2026-05-18T01:41:48.350049Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:41:48.350049Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"SsALifms4ArF3Doj7W02HOCRZLUQAr3Xh/S8D7+lMXQFQEuX73WkDVGHMAWOlxuutfSYooppAgRM+o7b9oSiBg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:41:48.350560Z","signed_message":"canonical_sha256_bytes"},"source_id":"1410.3883","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:08cf86d720cb89baa2aa95aa889256035fb4c08d1a16bc6c3f28eebbdb97285e","sha256:c149aee03b98d4c8622c0185a414422ba133edeab5b69d4291292689ae712457"],"state_sha256":"5a9d450c0f628a2391139920f7f338b4272c2d08cc0d72d57dd4b5efaef97231"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Y+uls3HpWOTbNPmfkFZjh8W1BXs4BtfL1aEwc8tLWJLMSmlIzY8iiMfuPjb5WkFJIERkWXknnoCYCQEUgBtQAQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T15:25:07.179742Z","bundle_sha256":"adf2695b11fc49164af0197dd16fcbd155388429b2477d4f4f2d94dcae33ed9e"}}