{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2025:YK3YHDX6GZDYSN427KKQMGNAGR","short_pith_number":"pith:YK3YHDX6","canonical_record":{"source":{"id":"2502.12914","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-02-18T14:55:03Z","cross_cats_sorted":[],"title_canon_sha256":"578f26718fd14f90f4056d02621a976d00741025bb0f289d038ab510298a75c5","abstract_canon_sha256":"97bdabf1ca28adfda3de760a27fff74392c5715338a67ceb8ca0c2ebd7ecd3a3"},"schema_version":"1.0"},"canonical_sha256":"c2b7838efe364789379afa950619a03466dc6d767079ec8b92d216d98b5e18a7","source":{"kind":"arxiv","id":"2502.12914","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2502.12914","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"arxiv_version","alias_value":"2502.12914v1","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.12914","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"pith_short_12","alias_value":"YK3YHDX6GZDY","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"pith_short_16","alias_value":"YK3YHDX6GZDYSN42","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"pith_short_8","alias_value":"YK3YHDX6","created_at":"2026-07-05T11:44:45Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2025:YK3YHDX6GZDYSN427KKQMGNAGR","target":"record","payload":{"canonical_record":{"source":{"id":"2502.12914","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-02-18T14:55:03Z","cross_cats_sorted":[],"title_canon_sha256":"578f26718fd14f90f4056d02621a976d00741025bb0f289d038ab510298a75c5","abstract_canon_sha256":"97bdabf1ca28adfda3de760a27fff74392c5715338a67ceb8ca0c2ebd7ecd3a3"},"schema_version":"1.0"},"canonical_sha256":"c2b7838efe364789379afa950619a03466dc6d767079ec8b92d216d98b5e18a7","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:44:45.458639Z","signature_b64":"GAAQo7A2tAZDEwZkDSc/BwLg2DdyhJLG3HLTfTUgKxCcaKsW+UiFFX+pTu+mLDR+L9yOo3EcLsNgybTfgxmdDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c2b7838efe364789379afa950619a03466dc6d767079ec8b92d216d98b5e18a7","last_reissued_at":"2026-07-05T11:44:45.458177Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:44:45.458177Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2502.12914","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":"2026-07-05T11:44:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1RLTxMQuYPfXnO9b5dRFP3kaoGPUidFZaye6Z2OaLJ6JivBzlOe+b+0YC19+GdpPqFqcFLys9vlhQyUXYFnMCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-19T15:50:26.023775Z"},"content_sha256":"8faed7823e1a6f29da0c427cb98cc91f10a5a7f68eadd40892d86dd48a3d9f54","schema_version":"1.0","event_id":"sha256:8faed7823e1a6f29da0c427cb98cc91f10a5a7f68eadd40892d86dd48a3d9f54"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2025:YK3YHDX6GZDYSN427KKQMGNAGR","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Selection Function of Clusters in Dark Energy Survey Year 3 Data from Cross-Matching with South Pole Telescope Detections","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Plazas Malag\\'on, A. Carnero Rosell, A. K. Romer, A. Palmese, A. Saro, B. Flaugher, B. Santiago, C. L. Reichardt, C. To, D. Brooks, D. Gruen, D. J. James, D. L. Hollowood, D. L. Tucker, D. Sanchez Cid, E. Gaztanaga, E. Sanchez, E. Suchyta, F. Andrade-Oliveira, G. Gutierrez, G. Tarle, H. T. Diehl, H.-Y. Wu, I. Sevilla-Noarbe, J. Carretero, J. Frieman, J. Garc\\'ia-Bellido, J. Hlacacek-Larrondo, J. J. Mohr, J. L. Marshall, J. Mena-Fern\\'andez, J. Weller, K. Honscheid, L. E. Bleem, L. N. da Costa, M. Aguena, M. Costanzi, M. E. S. Pereira, M. Klein, M. Smith, M. Soares-Santos, M. W. Sommer, N. Weaverdyck, P. Doel, P. Wiseman, R. A. Gruendl, R. Miquel, S. Allam, S. Bocquet, S. Desai, S. Everett, S. Grandis, S. R. Hinton, S. Samuroff, T. M. Davis","submitted_at":"2025-02-18T14:55:03Z","abstract_excerpt":"Galaxy clusters selected based on overdensities of galaxies in photometric surveys provide the largest cluster samples. Yet modeling the selection function of such samples is complicated by non-cluster members projected along the line of sight (projection effects) and the potential detection of unvirialized objects (contamination). We empirically constrain the magnitude of these effects by cross-matching galaxy clusters selected in the Dark Energy survey data with the \\rdmpr$\\,$ algorithm with significant detections in three South Pole Telescope surveys (SZ, pol-ECS, pol-500d). For matched clu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.12914","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/2502.12914/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-05T11:44:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ZcMXrR/DhTZLS1FHXHYk6K8XCqXM9A67avRF/CQzytgbmUd0kb0WcVkObVEwpe6OowRgp1MTwyq6Wq3wMDO8CQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-19T15:50:26.024161Z"},"content_sha256":"bb743a94c1f424432a82d7b8f0defe6c46dfb797dd9ba85d79f58aee4ce8be82","schema_version":"1.0","event_id":"sha256:bb743a94c1f424432a82d7b8f0defe6c46dfb797dd9ba85d79f58aee4ce8be82"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/YK3YHDX6GZDYSN427KKQMGNAGR/bundle.json","state_url":"https://pith.science/pith/YK3YHDX6GZDYSN427KKQMGNAGR/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/YK3YHDX6GZDYSN427KKQMGNAGR/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":"2026-08-19T15:50:26Z","links":{"resolver":"https://pith.science/pith/YK3YHDX6GZDYSN427KKQMGNAGR","bundle":"https://pith.science/pith/YK3YHDX6GZDYSN427KKQMGNAGR/bundle.json","state":"https://pith.science/pith/YK3YHDX6GZDYSN427KKQMGNAGR/state.json","well_known_bundle":"https://pith.science/.well-known/pith/YK3YHDX6GZDYSN427KKQMGNAGR/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2025:YK3YHDX6GZDYSN427KKQMGNAGR","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":"97bdabf1ca28adfda3de760a27fff74392c5715338a67ceb8ca0c2ebd7ecd3a3","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-02-18T14:55:03Z","title_canon_sha256":"578f26718fd14f90f4056d02621a976d00741025bb0f289d038ab510298a75c5"},"schema_version":"1.0","source":{"id":"2502.12914","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2502.12914","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"arxiv_version","alias_value":"2502.12914v1","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.12914","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"pith_short_12","alias_value":"YK3YHDX6GZDY","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"pith_short_16","alias_value":"YK3YHDX6GZDYSN42","created_at":"2026-07-05T11:44:45Z"},{"alias_kind":"pith_short_8","alias_value":"YK3YHDX6","created_at":"2026-07-05T11:44:45Z"}],"graph_snapshots":[{"event_id":"sha256:bb743a94c1f424432a82d7b8f0defe6c46dfb797dd9ba85d79f58aee4ce8be82","target":"graph","created_at":"2026-07-05T11:44:45Z","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"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/2502.12914/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"Galaxy clusters selected based on overdensities of galaxies in photometric surveys provide the largest cluster samples. Yet modeling the selection function of such samples is complicated by non-cluster members projected along the line of sight (projection effects) and the potential detection of unvirialized objects (contamination). We empirically constrain the magnitude of these effects by cross-matching galaxy clusters selected in the Dark Energy survey data with the \\rdmpr$\\,$ algorithm with significant detections in three South Pole Telescope surveys (SZ, pol-ECS, pol-500d). For matched clu","authors_text":"A. A. Plazas Malag\\'on, A. Carnero Rosell, A. K. Romer, A. Palmese, A. Saro, B. Flaugher, B. Santiago, C. L. Reichardt, C. To, D. Brooks, D. Gruen, D. J. James, D. L. Hollowood, D. L. Tucker, D. Sanchez Cid, E. Gaztanaga, E. Sanchez, E. Suchyta, F. Andrade-Oliveira, G. Gutierrez, G. Tarle, H. T. Diehl, H.-Y. Wu, I. Sevilla-Noarbe, J. Carretero, J. Frieman, J. Garc\\'ia-Bellido, J. Hlacacek-Larrondo, J. J. Mohr, J. L. Marshall, J. Mena-Fern\\'andez, J. Weller, K. Honscheid, L. E. Bleem, L. N. da Costa, M. Aguena, M. Costanzi, M. E. S. Pereira, M. Klein, M. Smith, M. Soares-Santos, M. W. Sommer, N. Weaverdyck, P. Doel, P. Wiseman, R. A. Gruendl, R. Miquel, S. Allam, S. Bocquet, S. Desai, S. Everett, S. Grandis, S. R. Hinton, S. Samuroff, T. M. Davis","cross_cats":[],"headline":"","license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-02-18T14:55:03Z","title":"Selection Function of Clusters in Dark Energy Survey Year 3 Data from Cross-Matching with South Pole Telescope Detections"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.12914","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":"sha256:8faed7823e1a6f29da0c427cb98cc91f10a5a7f68eadd40892d86dd48a3d9f54","target":"record","created_at":"2026-07-05T11:44:45Z","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":"97bdabf1ca28adfda3de760a27fff74392c5715338a67ceb8ca0c2ebd7ecd3a3","cross_cats_sorted":[],"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2025-02-18T14:55:03Z","title_canon_sha256":"578f26718fd14f90f4056d02621a976d00741025bb0f289d038ab510298a75c5"},"schema_version":"1.0","source":{"id":"2502.12914","kind":"arxiv","version":1}},"canonical_sha256":"c2b7838efe364789379afa950619a03466dc6d767079ec8b92d216d98b5e18a7","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"c2b7838efe364789379afa950619a03466dc6d767079ec8b92d216d98b5e18a7","first_computed_at":"2026-07-05T11:44:45.458177Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-05T11:44:45.458177Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"GAAQo7A2tAZDEwZkDSc/BwLg2DdyhJLG3HLTfTUgKxCcaKsW+UiFFX+pTu+mLDR+L9yOo3EcLsNgybTfgxmdDw==","signature_status":"signed_v1","signed_at":"2026-07-05T11:44:45.458639Z","signed_message":"canonical_sha256_bytes"},"source_id":"2502.12914","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:8faed7823e1a6f29da0c427cb98cc91f10a5a7f68eadd40892d86dd48a3d9f54","sha256:bb743a94c1f424432a82d7b8f0defe6c46dfb797dd9ba85d79f58aee4ce8be82"],"state_sha256":"27aa51e2ffff7709acdd32dfa68577489c646b35fe2b085da5c58c5df5997d03"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"u4um6h4jCXfE6oGSW1Q6j0RX6iRa0vQoF+pW6i9rq04hV7yPHIESK/jiJgG6DYfcBZdkngUoUTvQz2wfICc6BQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-19T15:50:26.026574Z","bundle_sha256":"349b40bf68b6d1f83b2b76df34b1ab47a8b439df9394ec6a9d2ec2fbcea0ff64"}}