{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:HQ4JCDCETHQXFWUZDLWDY4K377","short_pith_number":"pith:HQ4JCDCE","schema_version":"1.0","canonical_sha256":"3c38910c4499e172da991aec3c715bffeef0a192fe5b5f6bf945296f4f637458","source":{"kind":"arxiv","id":"2406.03535","version":1},"attestation_state":"computed","paper":{"title":"Any Way the Wind Blows: Quantifying Superbubbles and their Outflows in Simulated Galaxies across $z \\approx 0-3$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrew Wetzel, Blakesley Burkhart, Claude-Andr\\'e Faucher-Gigu\\`ere, Du\\v{s}an Kere\\v{s}, Lori E. Porter, Matthew E. Orr, Philip F. Hopkins","submitted_at":"2024-06-05T18:00:01Z","abstract_excerpt":"We present an investigation of clustered stellar feedback in the form of superbubbles identified within eleven galaxies from the FIRE-2 (Feedback in Realistic Environments) cosmological zoom-in simulation suite, at both cosmic noon (1 < z < 3) and in the local Universe. We study the spatially-resolved multiphase outflows that these supernovae drive, comparing our findings with recent theory and observations. These simulations consist of five LMC-mass galaxies and six Milky Way-mass progenitors (with a minimum baryonic particle mass of $m_{b.min} = 7100 M_{\\odot}$), for which we calculate the l"},"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":"2406.03535","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2024-06-05T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"a6f627e1283249fa3f6034ae5e3b8ddb09d03f845811bb9fc20ae229d739b597","abstract_canon_sha256":"f7899819f81fcdf93463345bbd45b7a31621679b31042a17943903c345d6fafc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:28:12.703478Z","signature_b64":"ND4fvrRc6bzDWO2/FH4VhBKQVuA7NurvfT8dR04sFmfmplP0Kw/INn7VNZjYsYaxAwRvTxdAj4caoByeqpRKDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3c38910c4499e172da991aec3c715bffeef0a192fe5b5f6bf945296f4f637458","last_reissued_at":"2026-07-05T08:28:12.703030Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:28:12.703030Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Any Way the Wind Blows: Quantifying Superbubbles and their Outflows in Simulated Galaxies across $z \\approx 0-3$","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Andrew Wetzel, Blakesley Burkhart, Claude-Andr\\'e Faucher-Gigu\\`ere, Du\\v{s}an Kere\\v{s}, Lori E. Porter, Matthew E. Orr, Philip F. Hopkins","submitted_at":"2024-06-05T18:00:01Z","abstract_excerpt":"We present an investigation of clustered stellar feedback in the form of superbubbles identified within eleven galaxies from the FIRE-2 (Feedback in Realistic Environments) cosmological zoom-in simulation suite, at both cosmic noon (1 < z < 3) and in the local Universe. We study the spatially-resolved multiphase outflows that these supernovae drive, comparing our findings with recent theory and observations. These simulations consist of five LMC-mass galaxies and six Milky Way-mass progenitors (with a minimum baryonic particle mass of $m_{b.min} = 7100 M_{\\odot}$), for which we calculate the l"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.03535","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2406.03535/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":"2406.03535","created_at":"2026-07-05T08:28:12.703096+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.03535v1","created_at":"2026-07-05T08:28:12.703096+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.03535","created_at":"2026-07-05T08:28:12.703096+00:00"},{"alias_kind":"pith_short_12","alias_value":"HQ4JCDCETHQX","created_at":"2026-07-05T08:28:12.703096+00:00"},{"alias_kind":"pith_short_16","alias_value":"HQ4JCDCETHQXFWUZ","created_at":"2026-07-05T08:28:12.703096+00:00"},{"alias_kind":"pith_short_8","alias_value":"HQ4JCDCE","created_at":"2026-07-05T08:28:12.703096+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377","json":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377.json","graph_json":"https://pith.science/api/pith-number/HQ4JCDCETHQXFWUZDLWDY4K377/graph.json","events_json":"https://pith.science/api/pith-number/HQ4JCDCETHQXFWUZDLWDY4K377/events.json","paper":"https://pith.science/paper/HQ4JCDCE"},"agent_actions":{"view_html":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377","download_json":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377.json","view_paper":"https://pith.science/paper/HQ4JCDCE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.03535&json=true","fetch_graph":"https://pith.science/api/pith-number/HQ4JCDCETHQXFWUZDLWDY4K377/graph.json","fetch_events":"https://pith.science/api/pith-number/HQ4JCDCETHQXFWUZDLWDY4K377/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377/action/storage_attestation","attest_author":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377/action/author_attestation","sign_citation":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377/action/citation_signature","submit_replication":"https://pith.science/pith/HQ4JCDCETHQXFWUZDLWDY4K377/action/replication_record"}},"created_at":"2026-07-05T08:28:12.703096+00:00","updated_at":"2026-07-05T08:28:12.703096+00:00"}