{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:RGY4WFVSH7G47OB4S6IPCU3Q7A","short_pith_number":"pith:RGY4WFVS","schema_version":"1.0","canonical_sha256":"89b1cb16b23fcdcfb83c9790f15370f8017b1ce4bc666b8b916c80a3db3ca38c","source":{"kind":"arxiv","id":"2305.14424","version":2},"attestation_state":"computed","paper":{"title":"Cloud Atlas: Navigating the Multiphase Landscape of Tempestuous Galactic Winds","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Brent Tan, Drummond B. Fielding","submitted_at":"2023-05-23T18:00:04Z","abstract_excerpt":"Galaxies comprise intricate networks of interdependent processes which together govern their evolution. Central among these are the multiplicity of feedback channels, which remain incompletely understood. One outstanding problem is the understanding and modeling of the multiphase nature of galactic winds, which play a crucial role in galaxy formation and evolution. We present the results of three dimensional magnetohydrodynamical tall box interstellar medium patch simulations with clustered supernova driven outflows. Fragmentation of the interstellar medium during superbubble breakout seeds th"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2305.14424","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-05-23T18:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"35dcd8d4fb3a636f901b097c54865e225ce6c82d56eeb67900ff0a310a610e4f","abstract_canon_sha256":"8de671c67c83565bd6c1dc8512b371c3f206c09fbe03ff2aef5e6e9873238256"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:21:41.990651Z","signature_b64":"NhnFCZW38D7q3WVSCqim+RWu/6dZsIazspXOlZG4g1FhFK/f9w2NzTkgmHi/fr7eFh+Ly17IZEOQluNJG624DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"89b1cb16b23fcdcfb83c9790f15370f8017b1ce4bc666b8b916c80a3db3ca38c","last_reissued_at":"2026-07-05T07:21:41.990182Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:21:41.990182Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cloud Atlas: Navigating the Multiphase Landscape of Tempestuous Galactic Winds","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Brent Tan, Drummond B. Fielding","submitted_at":"2023-05-23T18:00:04Z","abstract_excerpt":"Galaxies comprise intricate networks of interdependent processes which together govern their evolution. Central among these are the multiplicity of feedback channels, which remain incompletely understood. One outstanding problem is the understanding and modeling of the multiphase nature of galactic winds, which play a crucial role in galaxy formation and evolution. We present the results of three dimensional magnetohydrodynamical tall box interstellar medium patch simulations with clustered supernova driven outflows. Fragmentation of the interstellar medium during superbubble breakout seeds th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.14424","kind":"arxiv","version":2},"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/2305.14424/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"},"aliases":[{"alias_kind":"arxiv","alias_value":"2305.14424","created_at":"2026-07-05T07:21:41.990239+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.14424v2","created_at":"2026-07-05T07:21:41.990239+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.14424","created_at":"2026-07-05T07:21:41.990239+00:00"},{"alias_kind":"pith_short_12","alias_value":"RGY4WFVSH7G4","created_at":"2026-07-05T07:21:41.990239+00:00"},{"alias_kind":"pith_short_16","alias_value":"RGY4WFVSH7G47OB4","created_at":"2026-07-05T07:21:41.990239+00:00"},{"alias_kind":"pith_short_8","alias_value":"RGY4WFVS","created_at":"2026-07-05T07:21:41.990239+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.07741","citing_title":"Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\\alpha$ Surface Brightness Ratio","ref_index":221,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13154","citing_title":"From Clumps to Sheets: Geometry Controls the Temperature PDF of Multi-Phase Gas","ref_index":66,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A","json":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A.json","graph_json":"https://pith.science/api/pith-number/RGY4WFVSH7G47OB4S6IPCU3Q7A/graph.json","events_json":"https://pith.science/api/pith-number/RGY4WFVSH7G47OB4S6IPCU3Q7A/events.json","paper":"https://pith.science/paper/RGY4WFVS"},"agent_actions":{"view_html":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A","download_json":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A.json","view_paper":"https://pith.science/paper/RGY4WFVS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.14424&json=true","fetch_graph":"https://pith.science/api/pith-number/RGY4WFVSH7G47OB4S6IPCU3Q7A/graph.json","fetch_events":"https://pith.science/api/pith-number/RGY4WFVSH7G47OB4S6IPCU3Q7A/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A/action/storage_attestation","attest_author":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A/action/author_attestation","sign_citation":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A/action/citation_signature","submit_replication":"https://pith.science/pith/RGY4WFVSH7G47OB4S6IPCU3Q7A/action/replication_record"}},"created_at":"2026-07-05T07:21:41.990239+00:00","updated_at":"2026-07-05T07:21:41.990239+00:00"}