{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:F6NNMRF64755KOT6NXJR6MEJ3K","short_pith_number":"pith:F6NNMRF6","canonical_record":{"source":{"id":"1407.5729","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-22T05:12:13Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"16c89f5340e91a39425e562cc7d31c5b648b76decb84f2ca35574197b2cfe2b3","abstract_canon_sha256":"0f1afc3e86ddaf7c9ed07153c1f4c74bb267a5342a08daabaead3ea14ca9f773"},"schema_version":"1.0"},"canonical_sha256":"2f9ad644bee7fbd53a7e6dd31f3089daacdbb109628242a23e9aec910016a03f","source":{"kind":"arxiv","id":"1407.5729","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1407.5729","created_at":"2026-05-18T02:42:45Z"},{"alias_kind":"arxiv_version","alias_value":"1407.5729v1","created_at":"2026-05-18T02:42:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.5729","created_at":"2026-05-18T02:42:45Z"},{"alias_kind":"pith_short_12","alias_value":"F6NNMRF64755","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_16","alias_value":"F6NNMRF64755KOT6","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_8","alias_value":"F6NNMRF6","created_at":"2026-05-18T12:28:28Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:F6NNMRF64755KOT6NXJR6MEJ3K","target":"record","payload":{"canonical_record":{"source":{"id":"1407.5729","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-22T05:12:13Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"16c89f5340e91a39425e562cc7d31c5b648b76decb84f2ca35574197b2cfe2b3","abstract_canon_sha256":"0f1afc3e86ddaf7c9ed07153c1f4c74bb267a5342a08daabaead3ea14ca9f773"},"schema_version":"1.0"},"canonical_sha256":"2f9ad644bee7fbd53a7e6dd31f3089daacdbb109628242a23e9aec910016a03f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:42:45.822439Z","signature_b64":"CRI9yPk0Y8ufW6B4/tXbICKKR7cniOr2m31IVNK5wfVVRq9KUWhNp4GIwF8M71HIqNTz2uEzNianyw/lU8jiBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2f9ad644bee7fbd53a7e6dd31f3089daacdbb109628242a23e9aec910016a03f","last_reissued_at":"2026-05-18T02:42:45.821879Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:42:45.821879Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1407.5729","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":"2026-05-18T02:42:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"KS4toi/MhvGDgg/FMST75mjyb+BlFq7NW81KECymLmChG4Ym9HXUjZ88LoxSg7OGq/Cb1k9GakjmTH1SmiBUCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T19:03:50.894229Z"},"content_sha256":"468907e83b0631ba0c5ce6e61ae47797fc032d8269345bc8e0478ed1734f71e0","schema_version":"1.0","event_id":"sha256:468907e83b0631ba0c5ce6e61ae47797fc032d8269345bc8e0478ed1734f71e0"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:F6NNMRF64755KOT6NXJR6MEJ3K","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"Andrew Benson, Dominik Steinhauser, Florian Pranger, Harald H\\\"oller, Josef St\\\"ockl, Lorenzo Lovisari, Markus Haider","submitted_at":"2014-07-22T05:12:13Z","abstract_excerpt":"We present a simulation setup for studying the dynamical and chemical evolution of the intracluster medium (ICM) and analyze a sample of 12 galaxy clusters that are diverse both kinetically (pre-merger, merging, virialized) and in total mass (M vir = 1.17 x 10^14 - 1.06 x 10^15 M). We analyzed the metal mass fraction in the ICM as a function of redshift and discuss radial trends as well as projected 2D metallicity maps. The setup combines high mass resolution N-body simulations with the semi-analytical galaxy formation model Galacticus for consistent treatment of the subgrid physics (such as g"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.5729","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":"2026-05-18T02:42:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2gBHjgY2bvPhtGnEM/MM0BheaJPZa0/Yv/WBjyawYMDDc+rCzmzO/5RGSjoeWQTQRSZftFgyCzQWosqyjwBzCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T19:03:50.894593Z"},"content_sha256":"91df236af8414802c2b074bb3f7a3f9565fb3263ee3664961fd02a707a754a21","schema_version":"1.0","event_id":"sha256:91df236af8414802c2b074bb3f7a3f9565fb3263ee3664961fd02a707a754a21"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/F6NNMRF64755KOT6NXJR6MEJ3K/bundle.json","state_url":"https://pith.science/pith/F6NNMRF64755KOT6NXJR6MEJ3K/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/F6NNMRF64755KOT6NXJR6MEJ3K/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":"2026-06-03T19:03:50Z","links":{"resolver":"https://pith.science/pith/F6NNMRF64755KOT6NXJR6MEJ3K","bundle":"https://pith.science/pith/F6NNMRF64755KOT6NXJR6MEJ3K/bundle.json","state":"https://pith.science/pith/F6NNMRF64755KOT6NXJR6MEJ3K/state.json","well_known_bundle":"https://pith.science/.well-known/pith/F6NNMRF64755KOT6NXJR6MEJ3K/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:F6NNMRF64755KOT6NXJR6MEJ3K","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":"0f1afc3e86ddaf7c9ed07153c1f4c74bb267a5342a08daabaead3ea14ca9f773","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-22T05:12:13Z","title_canon_sha256":"16c89f5340e91a39425e562cc7d31c5b648b76decb84f2ca35574197b2cfe2b3"},"schema_version":"1.0","source":{"id":"1407.5729","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1407.5729","created_at":"2026-05-18T02:42:45Z"},{"alias_kind":"arxiv_version","alias_value":"1407.5729v1","created_at":"2026-05-18T02:42:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1407.5729","created_at":"2026-05-18T02:42:45Z"},{"alias_kind":"pith_short_12","alias_value":"F6NNMRF64755","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_16","alias_value":"F6NNMRF64755KOT6","created_at":"2026-05-18T12:28:28Z"},{"alias_kind":"pith_short_8","alias_value":"F6NNMRF6","created_at":"2026-05-18T12:28:28Z"}],"graph_snapshots":[{"event_id":"sha256:91df236af8414802c2b074bb3f7a3f9565fb3263ee3664961fd02a707a754a21","target":"graph","created_at":"2026-05-18T02:42:45Z","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"},"paper":{"abstract_excerpt":"We present a simulation setup for studying the dynamical and chemical evolution of the intracluster medium (ICM) and analyze a sample of 12 galaxy clusters that are diverse both kinetically (pre-merger, merging, virialized) and in total mass (M vir = 1.17 x 10^14 - 1.06 x 10^15 M). We analyzed the metal mass fraction in the ICM as a function of redshift and discuss radial trends as well as projected 2D metallicity maps. The setup combines high mass resolution N-body simulations with the semi-analytical galaxy formation model Galacticus for consistent treatment of the subgrid physics (such as g","authors_text":"Andrew Benson, Dominik Steinhauser, Florian Pranger, Harald H\\\"oller, Josef St\\\"ockl, Lorenzo Lovisari, Markus Haider","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-22T05:12:13Z","title":"Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1407.5729","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":"sha256:468907e83b0631ba0c5ce6e61ae47797fc032d8269345bc8e0478ed1734f71e0","target":"record","created_at":"2026-05-18T02:42:45Z","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":"0f1afc3e86ddaf7c9ed07153c1f4c74bb267a5342a08daabaead3ea14ca9f773","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2014-07-22T05:12:13Z","title_canon_sha256":"16c89f5340e91a39425e562cc7d31c5b648b76decb84f2ca35574197b2cfe2b3"},"schema_version":"1.0","source":{"id":"1407.5729","kind":"arxiv","version":1}},"canonical_sha256":"2f9ad644bee7fbd53a7e6dd31f3089daacdbb109628242a23e9aec910016a03f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"2f9ad644bee7fbd53a7e6dd31f3089daacdbb109628242a23e9aec910016a03f","first_computed_at":"2026-05-18T02:42:45.821879Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:42:45.821879Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"CRI9yPk0Y8ufW6B4/tXbICKKR7cniOr2m31IVNK5wfVVRq9KUWhNp4GIwF8M71HIqNTz2uEzNianyw/lU8jiBQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:42:45.822439Z","signed_message":"canonical_sha256_bytes"},"source_id":"1407.5729","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:468907e83b0631ba0c5ce6e61ae47797fc032d8269345bc8e0478ed1734f71e0","sha256:91df236af8414802c2b074bb3f7a3f9565fb3263ee3664961fd02a707a754a21"],"state_sha256":"d1d08e5c9205c837452980f102681a24d4b6301deb986e96002e47aa72c32db4"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"bhX3cQl/nB8z7TCIyc9cQbBr0kWJ2ROIdO2W34TMafYGz21ahR/Nyo6/BsP0nSsFGJo2oO1FiFjP7IeQpdeLDg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-03T19:03:50.896719Z","bundle_sha256":"245fe33842f82fdeed3641a03aa51f6cad63293d6a858ebac3f7bba3d28a07e8"}}