{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2009:47Q6B4RMSEQQ3XLHZCY6NUXJPC","short_pith_number":"pith:47Q6B4RM","canonical_record":{"source":{"id":"0910.4958","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-10-26T19:06:45Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"c65289f11a892ddd7ed0365548c45a5a7ccc80ff30b1488c782d475674df7ea4","abstract_canon_sha256":"54119770912d7e6ac338b0b1e22bf665399e192f4ca23b9070ed3f8595f7d56b"},"schema_version":"1.0"},"canonical_sha256":"e7e1e0f22c91210ddd67c8b1e6d2e978a139de0eda1dc5fc4cdcaf154f050336","source":{"kind":"arxiv","id":"0910.4958","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"0910.4958","created_at":"2026-05-18T04:29:35Z"},{"alias_kind":"arxiv_version","alias_value":"0910.4958v3","created_at":"2026-05-18T04:29:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0910.4958","created_at":"2026-05-18T04:29:35Z"},{"alias_kind":"pith_short_12","alias_value":"47Q6B4RMSEQQ","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_16","alias_value":"47Q6B4RMSEQQ3XLH","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_8","alias_value":"47Q6B4RM","created_at":"2026-05-18T12:25:58Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2009:47Q6B4RMSEQQ3XLHZCY6NUXJPC","target":"record","payload":{"canonical_record":{"source":{"id":"0910.4958","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-10-26T19:06:45Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"c65289f11a892ddd7ed0365548c45a5a7ccc80ff30b1488c782d475674df7ea4","abstract_canon_sha256":"54119770912d7e6ac338b0b1e22bf665399e192f4ca23b9070ed3f8595f7d56b"},"schema_version":"1.0"},"canonical_sha256":"e7e1e0f22c91210ddd67c8b1e6d2e978a139de0eda1dc5fc4cdcaf154f050336","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:29:35.167955Z","signature_b64":"QzIXC0bcLCMUCsMM7l+YVEuzxRFrBZ7oqQijSL6zE3pNxPqzwf7wB1XczADIMaGLMgHCaF+QRM4BAJdFzxeyAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7e1e0f22c91210ddd67c8b1e6d2e978a139de0eda1dc5fc4cdcaf154f050336","last_reissued_at":"2026-05-18T04:29:35.167482Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:29:35.167482Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"0910.4958","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":"2026-05-18T04:29:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"5AKiY/K8f/M0wvku0SHuC+4WoTUSHsX0hWL9XP7ph4TjR4m4c+iQzWH08cnIej5g8Ty+QT38A9/Htx7AWcLcBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T00:38:35.116919Z"},"content_sha256":"d793182b4421aa625f85c53281bc593be4de32f0730edf09c308f2d1e3064d75","schema_version":"1.0","event_id":"sha256:d793182b4421aa625f85c53281bc593be4de32f0730edf09c308f2d1e3064d75"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2009:47Q6B4RMSEQQ3XLHZCY6NUXJPC","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A new measurement of the bulk flow of X-ray luminous clusters of galaxies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"A. Edge (U of Durham, A. Kashlinsky (GSFC), D. Kocevski (UCD), F. Atrio-Barandela (U Salamanca, Hawaii), H. Ebeling (IfA, Spain), UK)","submitted_at":"2009-10-26T19:06:45Z","abstract_excerpt":"We present new measurements of the large-scale bulk flows of galaxy clusters based on 5-year WMAP data and a significantly expanded X-ray cluster catalogue. Our method probes the flow via measurements of the kinematic Sunyaev-Zeldovich (SZ) effect produced by the hot gas in moving clusters. It computes the dipole in the cosmic microwave background (CMB) data at cluster pixels, which preserves the SZ component while integrating down other contributions. Our improved catalog of over 1,000 clusters enables us to further investigate possible systematic effects and, thanks to a higher median cluste"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0910.4958","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":"2026-05-18T04:29:35Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"1mT4beAPGrswgbyX0+6DVdWlcn7VyahOfaza1VPjf6d77KgfdtuL3YA4YFTdsUBUuJtuOf2oYJIDN0J2qav8Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T00:38:35.117586Z"},"content_sha256":"d739f671b2a39c7499bd056673352a8a531529c1df0efb3a1a85ad77a62607db","schema_version":"1.0","event_id":"sha256:d739f671b2a39c7499bd056673352a8a531529c1df0efb3a1a85ad77a62607db"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/47Q6B4RMSEQQ3XLHZCY6NUXJPC/bundle.json","state_url":"https://pith.science/pith/47Q6B4RMSEQQ3XLHZCY6NUXJPC/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/47Q6B4RMSEQQ3XLHZCY6NUXJPC/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":"2026-05-26T00:38:35Z","links":{"resolver":"https://pith.science/pith/47Q6B4RMSEQQ3XLHZCY6NUXJPC","bundle":"https://pith.science/pith/47Q6B4RMSEQQ3XLHZCY6NUXJPC/bundle.json","state":"https://pith.science/pith/47Q6B4RMSEQQ3XLHZCY6NUXJPC/state.json","well_known_bundle":"https://pith.science/.well-known/pith/47Q6B4RMSEQQ3XLHZCY6NUXJPC/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2009:47Q6B4RMSEQQ3XLHZCY6NUXJPC","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":"54119770912d7e6ac338b0b1e22bf665399e192f4ca23b9070ed3f8595f7d56b","cross_cats_sorted":["hep-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-10-26T19:06:45Z","title_canon_sha256":"c65289f11a892ddd7ed0365548c45a5a7ccc80ff30b1488c782d475674df7ea4"},"schema_version":"1.0","source":{"id":"0910.4958","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"0910.4958","created_at":"2026-05-18T04:29:35Z"},{"alias_kind":"arxiv_version","alias_value":"0910.4958v3","created_at":"2026-05-18T04:29:35Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0910.4958","created_at":"2026-05-18T04:29:35Z"},{"alias_kind":"pith_short_12","alias_value":"47Q6B4RMSEQQ","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_16","alias_value":"47Q6B4RMSEQQ3XLH","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_8","alias_value":"47Q6B4RM","created_at":"2026-05-18T12:25:58Z"}],"graph_snapshots":[{"event_id":"sha256:d739f671b2a39c7499bd056673352a8a531529c1df0efb3a1a85ad77a62607db","target":"graph","created_at":"2026-05-18T04:29:35Z","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":"We present new measurements of the large-scale bulk flows of galaxy clusters based on 5-year WMAP data and a significantly expanded X-ray cluster catalogue. Our method probes the flow via measurements of the kinematic Sunyaev-Zeldovich (SZ) effect produced by the hot gas in moving clusters. It computes the dipole in the cosmic microwave background (CMB) data at cluster pixels, which preserves the SZ component while integrating down other contributions. Our improved catalog of over 1,000 clusters enables us to further investigate possible systematic effects and, thanks to a higher median cluste","authors_text":"A. Edge (U of Durham, A. Kashlinsky (GSFC), D. Kocevski (UCD), F. Atrio-Barandela (U Salamanca, Hawaii), H. Ebeling (IfA, Spain), UK)","cross_cats":["hep-ph"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-10-26T19:06:45Z","title":"A new measurement of the bulk flow of X-ray luminous clusters of galaxies"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0910.4958","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:d793182b4421aa625f85c53281bc593be4de32f0730edf09c308f2d1e3064d75","target":"record","created_at":"2026-05-18T04:29:35Z","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":"54119770912d7e6ac338b0b1e22bf665399e192f4ca23b9070ed3f8595f7d56b","cross_cats_sorted":["hep-ph"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-10-26T19:06:45Z","title_canon_sha256":"c65289f11a892ddd7ed0365548c45a5a7ccc80ff30b1488c782d475674df7ea4"},"schema_version":"1.0","source":{"id":"0910.4958","kind":"arxiv","version":3}},"canonical_sha256":"e7e1e0f22c91210ddd67c8b1e6d2e978a139de0eda1dc5fc4cdcaf154f050336","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"e7e1e0f22c91210ddd67c8b1e6d2e978a139de0eda1dc5fc4cdcaf154f050336","first_computed_at":"2026-05-18T04:29:35.167482Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:29:35.167482Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"QzIXC0bcLCMUCsMM7l+YVEuzxRFrBZ7oqQijSL6zE3pNxPqzwf7wB1XczADIMaGLMgHCaF+QRM4BAJdFzxeyAg==","signature_status":"signed_v1","signed_at":"2026-05-18T04:29:35.167955Z","signed_message":"canonical_sha256_bytes"},"source_id":"0910.4958","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:d793182b4421aa625f85c53281bc593be4de32f0730edf09c308f2d1e3064d75","sha256:d739f671b2a39c7499bd056673352a8a531529c1df0efb3a1a85ad77a62607db"],"state_sha256":"be0e66d6026bf52059cd63e4150f5f31cba4780de1086525125f97deb3c046b9"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"bypSKyrgmW3sP8E5YmVyfxzvZkbrRD5AAe6g/KqNBgVHXGfMGeV4S2O4NP/+RLPjpkuIWSuiKBgWdwW2/bJnAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T00:38:35.122200Z","bundle_sha256":"a6cef639b64556b570cd78e20dd1b7556a342672cf2f71759f1acfdcf7b5507d"}}