{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:TL6JM36IRC5YFYIH2M6MU557BQ","short_pith_number":"pith:TL6JM36I","canonical_record":{"source":{"id":"1009.3305","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-17T00:48:14Z","cross_cats_sorted":[],"title_canon_sha256":"c9e0c19b2fc6ff9ba9fa8b20656efba6f7d9d43c5b64fe9d3cf2d9a876843c2b","abstract_canon_sha256":"9bb5a6d76c686f217ab5c09ae1c2402c8e0a09fc89c33fcceda7638a7a391712"},"schema_version":"1.0"},"canonical_sha256":"9afc966fc888bb82e107d33cca77bf0c2d13a305be64e9fd1b088449711b234b","source":{"kind":"arxiv","id":"1009.3305","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1009.3305","created_at":"2026-05-18T02:05:25Z"},{"alias_kind":"arxiv_version","alias_value":"1009.3305v1","created_at":"2026-05-18T02:05:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.3305","created_at":"2026-05-18T02:05:25Z"},{"alias_kind":"pith_short_12","alias_value":"TL6JM36IRC5Y","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_16","alias_value":"TL6JM36IRC5YFYIH","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_8","alias_value":"TL6JM36I","created_at":"2026-05-18T12:26:13Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:TL6JM36IRC5YFYIH2M6MU557BQ","target":"record","payload":{"canonical_record":{"source":{"id":"1009.3305","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-17T00:48:14Z","cross_cats_sorted":[],"title_canon_sha256":"c9e0c19b2fc6ff9ba9fa8b20656efba6f7d9d43c5b64fe9d3cf2d9a876843c2b","abstract_canon_sha256":"9bb5a6d76c686f217ab5c09ae1c2402c8e0a09fc89c33fcceda7638a7a391712"},"schema_version":"1.0"},"canonical_sha256":"9afc966fc888bb82e107d33cca77bf0c2d13a305be64e9fd1b088449711b234b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:25.271847Z","signature_b64":"+NBqBQQrCF6VLNY9HJmPoD73VpW/Q/7+FPVwwNJlBZ/Bgqi1xdQhD49M/m9JWP/NB1uxKYtxnQnwktporcbeAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9afc966fc888bb82e107d33cca77bf0c2d13a305be64e9fd1b088449711b234b","last_reissued_at":"2026-05-18T02:05:25.271179Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:25.271179Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1009.3305","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":"2026-05-18T02:05:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"428bjsKq3NtnaZvJaKlongBhuU4//bq7UZPxA6SBqeRmQBZbFAJze2EViMrQA7psqcxy8gpUI4ySx2Zg0axrDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-08T20:27:28.354509Z"},"content_sha256":"247ed584df1301b20ac4b00b8de1964dae2a240de124abbe7c534fe769e3e171","schema_version":"1.0","event_id":"sha256:247ed584df1301b20ac4b00b8de1964dae2a240de124abbe7c534fe769e3e171"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:TL6JM36IRC5YFYIH2M6MU557BQ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"An analysis of the temperature structure of galaxy clusters by means of the thermal Sunyaev-Zel'dovich effect","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"D. A. Prokhorov, S. Nagataki, Y. Dubois","submitted_at":"2010-09-17T00:48:14Z","abstract_excerpt":"Measurements of the Sunyaev-Zel'dovich (hereafter SZ) effect distortion of the cosmic microwave background provide us with an independent method to derive the gas temperature of galaxy clusters. In merging galaxy clusters the gas distribution is inhomogeneous and, therefore, the method of temperature measuring based on the SZ effect should be more relevant than that based on an X-ray emission analysis. Here we study a method for measuring the gas temperature in merging clusters by means of the SZ effect.\n  Our calculations of intensity maps of the SZ effect include relativistic corrections con"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.3305","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":"2026-05-18T02:05:25Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"kZin4MkB7BiluiF30vjwjuTTH0+oOfj/76KZO9imLwwZ6FWsrYUutuK9JmkNw04PABSdW+9c0MU1Zg1CW9nrDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-08T20:27:28.355247Z"},"content_sha256":"267c32e61e081254f56e63acf5f34245ea150ea7d73b01a2a217e5fe609d966e","schema_version":"1.0","event_id":"sha256:267c32e61e081254f56e63acf5f34245ea150ea7d73b01a2a217e5fe609d966e"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/TL6JM36IRC5YFYIH2M6MU557BQ/bundle.json","state_url":"https://pith.science/pith/TL6JM36IRC5YFYIH2M6MU557BQ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/TL6JM36IRC5YFYIH2M6MU557BQ/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":"2026-06-08T20:27:28Z","links":{"resolver":"https://pith.science/pith/TL6JM36IRC5YFYIH2M6MU557BQ","bundle":"https://pith.science/pith/TL6JM36IRC5YFYIH2M6MU557BQ/bundle.json","state":"https://pith.science/pith/TL6JM36IRC5YFYIH2M6MU557BQ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/TL6JM36IRC5YFYIH2M6MU557BQ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:TL6JM36IRC5YFYIH2M6MU557BQ","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":"9bb5a6d76c686f217ab5c09ae1c2402c8e0a09fc89c33fcceda7638a7a391712","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-17T00:48:14Z","title_canon_sha256":"c9e0c19b2fc6ff9ba9fa8b20656efba6f7d9d43c5b64fe9d3cf2d9a876843c2b"},"schema_version":"1.0","source":{"id":"1009.3305","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1009.3305","created_at":"2026-05-18T02:05:25Z"},{"alias_kind":"arxiv_version","alias_value":"1009.3305v1","created_at":"2026-05-18T02:05:25Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.3305","created_at":"2026-05-18T02:05:25Z"},{"alias_kind":"pith_short_12","alias_value":"TL6JM36IRC5Y","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_16","alias_value":"TL6JM36IRC5YFYIH","created_at":"2026-05-18T12:26:13Z"},{"alias_kind":"pith_short_8","alias_value":"TL6JM36I","created_at":"2026-05-18T12:26:13Z"}],"graph_snapshots":[{"event_id":"sha256:267c32e61e081254f56e63acf5f34245ea150ea7d73b01a2a217e5fe609d966e","target":"graph","created_at":"2026-05-18T02:05:25Z","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":"Measurements of the Sunyaev-Zel'dovich (hereafter SZ) effect distortion of the cosmic microwave background provide us with an independent method to derive the gas temperature of galaxy clusters. In merging galaxy clusters the gas distribution is inhomogeneous and, therefore, the method of temperature measuring based on the SZ effect should be more relevant than that based on an X-ray emission analysis. Here we study a method for measuring the gas temperature in merging clusters by means of the SZ effect.\n  Our calculations of intensity maps of the SZ effect include relativistic corrections con","authors_text":"D. A. Prokhorov, S. Nagataki, Y. Dubois","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-17T00:48:14Z","title":"An analysis of the temperature structure of galaxy clusters by means of the thermal Sunyaev-Zel'dovich effect"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.3305","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":"sha256:247ed584df1301b20ac4b00b8de1964dae2a240de124abbe7c534fe769e3e171","target":"record","created_at":"2026-05-18T02:05:25Z","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":"9bb5a6d76c686f217ab5c09ae1c2402c8e0a09fc89c33fcceda7638a7a391712","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-09-17T00:48:14Z","title_canon_sha256":"c9e0c19b2fc6ff9ba9fa8b20656efba6f7d9d43c5b64fe9d3cf2d9a876843c2b"},"schema_version":"1.0","source":{"id":"1009.3305","kind":"arxiv","version":1}},"canonical_sha256":"9afc966fc888bb82e107d33cca77bf0c2d13a305be64e9fd1b088449711b234b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"9afc966fc888bb82e107d33cca77bf0c2d13a305be64e9fd1b088449711b234b","first_computed_at":"2026-05-18T02:05:25.271179Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:05:25.271179Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"+NBqBQQrCF6VLNY9HJmPoD73VpW/Q/7+FPVwwNJlBZ/Bgqi1xdQhD49M/m9JWP/NB1uxKYtxnQnwktporcbeAg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:05:25.271847Z","signed_message":"canonical_sha256_bytes"},"source_id":"1009.3305","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:247ed584df1301b20ac4b00b8de1964dae2a240de124abbe7c534fe769e3e171","sha256:267c32e61e081254f56e63acf5f34245ea150ea7d73b01a2a217e5fe609d966e"],"state_sha256":"8352f97b785dd8091e31c1e5568797d00ce63bff383c8b9cb9f5ff8296f20b22"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"vc7DS0NYXeKpdAxjnBKFQiZmUkHdnSyyMS1kN75ZI+TSlEnD+2YeWsnktOG2FvYjkpzMOmi9AnqZOHmKSYAuDQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-08T20:27:28.358789Z","bundle_sha256":"0b744470486779b5857e841aa4f70ee9844675398486fd92f4dfd8aa23c13a19"}}