{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:ANPX3YGN7PKJ2C2CXSIF2ZWA6N","short_pith_number":"pith:ANPX3YGN","canonical_record":{"source":{"id":"1006.4760","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-24T11:54:01Z","cross_cats_sorted":[],"title_canon_sha256":"0dcce7ac27d01f7ae9ac6779d4b5738dff01bd85af67b98cde2429e5c333c667","abstract_canon_sha256":"05c5ec5096f38ce1b43ab1b55ea547c0bae9bbd008580314961e7c5fc31d971d"},"schema_version":"1.0"},"canonical_sha256":"035f7de0cdfbd49d0b42bc905d66c0f35ae4edd728152de33447794744f3267f","source":{"kind":"arxiv","id":"1006.4760","version":4},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.4760","created_at":"2026-05-18T02:06:42Z"},{"alias_kind":"arxiv_version","alias_value":"1006.4760v4","created_at":"2026-05-18T02:06:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.4760","created_at":"2026-05-18T02:06:42Z"},{"alias_kind":"pith_short_12","alias_value":"ANPX3YGN7PKJ","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_16","alias_value":"ANPX3YGN7PKJ2C2C","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_8","alias_value":"ANPX3YGN","created_at":"2026-05-18T12:26:05Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:ANPX3YGN7PKJ2C2CXSIF2ZWA6N","target":"record","payload":{"canonical_record":{"source":{"id":"1006.4760","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-24T11:54:01Z","cross_cats_sorted":[],"title_canon_sha256":"0dcce7ac27d01f7ae9ac6779d4b5738dff01bd85af67b98cde2429e5c333c667","abstract_canon_sha256":"05c5ec5096f38ce1b43ab1b55ea547c0bae9bbd008580314961e7c5fc31d971d"},"schema_version":"1.0"},"canonical_sha256":"035f7de0cdfbd49d0b42bc905d66c0f35ae4edd728152de33447794744f3267f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:42.807379Z","signature_b64":"jPaIrB/aEPpSO8SxpZ2018rP5kSem3ez69tlm8rat1ko7Ku0QT2frlzTAw5no8GVXtglxSOJ7zChIgkIOW0dDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"035f7de0cdfbd49d0b42bc905d66c0f35ae4edd728152de33447794744f3267f","last_reissued_at":"2026-05-18T02:06:42.806859Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:42.806859Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1006.4760","source_version":4,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T02:06:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"N0mjdL9KSSAgCUmkS+4ZooOjXFMIitB57lF6zNXwKJ7+fnWLKSep7ipUuEVmqvb1kmDkTT182MtDZlDa+JRWDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T08:40:11.110846Z"},"content_sha256":"3e7ea18fc3b45e2c5fa4c89f55b1c82fa908583a862e3af462f75fe06fc8dd01","schema_version":"1.0","event_id":"sha256:3e7ea18fc3b45e2c5fa4c89f55b1c82fa908583a862e3af462f75fe06fc8dd01"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:ANPX3YGN7PKJ2C2CXSIF2ZWA6N","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Frank C. van den Bosch, H. J. Mo, Ran Li, Xiaohu Yang, Zuhui Fan","submitted_at":"2010-06-24T11:54:01Z","abstract_excerpt":"We investigate the potential of exploiting the Sunyaev-Zeldovich effect (SZE) to study the properties of hot gas in galaxy groups. It is shown that, with upcoming SZE surveys, one can stack SZE maps around galaxy groups of similar halo masses selected from large galaxy redshift surveys to study the hot gas in halos represented by galaxy groups. We use various models for the hot halo gas to study how the expected SZE signals are affected by gas fraction, equation of state, halo concentration, and cosmology. Comparing the model predictions with the sensitivities expected from the SPT, ACT and Pl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.4760","kind":"arxiv","version":4},"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":"2026-05-18T02:06:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"iDlLuwpLpMs970H8sQmG1Wu8EqKalVYPrbHuJj735fXbwlzxRWCWq9E7DznJtyNJgxJaVjgdl2kIbpKU1XN3Bw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T08:40:11.111197Z"},"content_sha256":"61a146fc71af9b550298d52761440fc96b31e0bfe52bc0dd67491ec56a76920d","schema_version":"1.0","event_id":"sha256:61a146fc71af9b550298d52761440fc96b31e0bfe52bc0dd67491ec56a76920d"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/ANPX3YGN7PKJ2C2CXSIF2ZWA6N/bundle.json","state_url":"https://pith.science/pith/ANPX3YGN7PKJ2C2CXSIF2ZWA6N/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/ANPX3YGN7PKJ2C2CXSIF2ZWA6N/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":"2026-06-01T08:40:11Z","links":{"resolver":"https://pith.science/pith/ANPX3YGN7PKJ2C2CXSIF2ZWA6N","bundle":"https://pith.science/pith/ANPX3YGN7PKJ2C2CXSIF2ZWA6N/bundle.json","state":"https://pith.science/pith/ANPX3YGN7PKJ2C2CXSIF2ZWA6N/state.json","well_known_bundle":"https://pith.science/.well-known/pith/ANPX3YGN7PKJ2C2CXSIF2ZWA6N/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:ANPX3YGN7PKJ2C2CXSIF2ZWA6N","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":"05c5ec5096f38ce1b43ab1b55ea547c0bae9bbd008580314961e7c5fc31d971d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-24T11:54:01Z","title_canon_sha256":"0dcce7ac27d01f7ae9ac6779d4b5738dff01bd85af67b98cde2429e5c333c667"},"schema_version":"1.0","source":{"id":"1006.4760","kind":"arxiv","version":4}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1006.4760","created_at":"2026-05-18T02:06:42Z"},{"alias_kind":"arxiv_version","alias_value":"1006.4760v4","created_at":"2026-05-18T02:06:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.4760","created_at":"2026-05-18T02:06:42Z"},{"alias_kind":"pith_short_12","alias_value":"ANPX3YGN7PKJ","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_16","alias_value":"ANPX3YGN7PKJ2C2C","created_at":"2026-05-18T12:26:05Z"},{"alias_kind":"pith_short_8","alias_value":"ANPX3YGN","created_at":"2026-05-18T12:26:05Z"}],"graph_snapshots":[{"event_id":"sha256:61a146fc71af9b550298d52761440fc96b31e0bfe52bc0dd67491ec56a76920d","target":"graph","created_at":"2026-05-18T02:06:42Z","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 investigate the potential of exploiting the Sunyaev-Zeldovich effect (SZE) to study the properties of hot gas in galaxy groups. It is shown that, with upcoming SZE surveys, one can stack SZE maps around galaxy groups of similar halo masses selected from large galaxy redshift surveys to study the hot gas in halos represented by galaxy groups. We use various models for the hot halo gas to study how the expected SZE signals are affected by gas fraction, equation of state, halo concentration, and cosmology. Comparing the model predictions with the sensitivities expected from the SPT, ACT and Pl","authors_text":"Frank C. van den Bosch, H. J. Mo, Ran Li, Xiaohu Yang, Zuhui Fan","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-24T11:54:01Z","title":"Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.4760","kind":"arxiv","version":4},"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":"sha256:3e7ea18fc3b45e2c5fa4c89f55b1c82fa908583a862e3af462f75fe06fc8dd01","target":"record","created_at":"2026-05-18T02:06:42Z","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":"05c5ec5096f38ce1b43ab1b55ea547c0bae9bbd008580314961e7c5fc31d971d","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-24T11:54:01Z","title_canon_sha256":"0dcce7ac27d01f7ae9ac6779d4b5738dff01bd85af67b98cde2429e5c333c667"},"schema_version":"1.0","source":{"id":"1006.4760","kind":"arxiv","version":4}},"canonical_sha256":"035f7de0cdfbd49d0b42bc905d66c0f35ae4edd728152de33447794744f3267f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"035f7de0cdfbd49d0b42bc905d66c0f35ae4edd728152de33447794744f3267f","first_computed_at":"2026-05-18T02:06:42.806859Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:06:42.806859Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"jPaIrB/aEPpSO8SxpZ2018rP5kSem3ez69tlm8rat1ko7Ku0QT2frlzTAw5no8GVXtglxSOJ7zChIgkIOW0dDg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:06:42.807379Z","signed_message":"canonical_sha256_bytes"},"source_id":"1006.4760","source_kind":"arxiv","source_version":4}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3e7ea18fc3b45e2c5fa4c89f55b1c82fa908583a862e3af462f75fe06fc8dd01","sha256:61a146fc71af9b550298d52761440fc96b31e0bfe52bc0dd67491ec56a76920d"],"state_sha256":"c9e7700a7fddbeda03c8f68ae7e3c5ff0e61078291762d773ae8e01312f6d655"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Fa/DSmaCK49LSOmrh6z7j23ooDX9Ff0Gl/R5d8BsBU2GhgRQIe5PrDZLKdFfPUFh5PmmlC5+DX0lJObIFxXEDg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T08:40:11.113125Z","bundle_sha256":"84d4b48693a5857695e7b7bb060c06234e712f6a56b8ce70f6ee7eee9cbb0177"}}