{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:VB3OBRRZ3NLQI7WD4BX4PTDXNM","short_pith_number":"pith:VB3OBRRZ","schema_version":"1.0","canonical_sha256":"a876e0c639db57047ec3e06fc7cc776b18d66514a1924b276213ba870a81d4d1","source":{"kind":"arxiv","id":"1708.07341","version":1},"attestation_state":"computed","paper":{"title":"Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Avery Meiksin (IfA, Claudio Dalla Vecchia (Inst. Astrof. de Canarias, Jan-Pieter Paardekooper (U. Heidelberg), Sadegh Khochfar (IfA, Saul Kohn (U. Pennsylvania), U. de La Laguna), U. Edinburgh)","submitted_at":"2017-08-24T09:59:37Z","abstract_excerpt":"The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure-driven wind and a superbubble model, and a 3D cosmological simulation including gas dynamics from the First Billion Years (FiBY) project. The analytic models are normalized to match the diffuse X-ray emissivity of star-forming galaxies in the nearby Universe. The cosmological simulation uses physically motivated star formation and wind prescriptions, and includes radiative transfer corrections. The models and the simulation all are found to produ"},"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":"1708.07341","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2017-08-24T09:59:37Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"867ae4863390e68602d21860f5e1b7f5855641303e9d81b1895d5b350b2d95c9","abstract_canon_sha256":"043b52d850408d54cee9ce3ab4d2ecc5361c33b5b7d28341fa85ed714db7ba9f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:36:27.730992Z","signature_b64":"VDeqBa3H7tFdz3ba90XuyKMr2n+nQdD2mi8iNhyRnXr46/MaWRt9U193gX9dh0mYMqCtSwju/0joy/nsOIHeAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a876e0c639db57047ec3e06fc7cc776b18d66514a1924b276213ba870a81d4d1","last_reissued_at":"2026-05-18T00:36:27.730395Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:36:27.730395Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Avery Meiksin (IfA, Claudio Dalla Vecchia (Inst. Astrof. de Canarias, Jan-Pieter Paardekooper (U. Heidelberg), Sadegh Khochfar (IfA, Saul Kohn (U. Pennsylvania), U. de La Laguna), U. Edinburgh)","submitted_at":"2017-08-24T09:59:37Z","abstract_excerpt":"The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure-driven wind and a superbubble model, and a 3D cosmological simulation including gas dynamics from the First Billion Years (FiBY) project. The analytic models are normalized to match the diffuse X-ray emissivity of star-forming galaxies in the nearby Universe. The cosmological simulation uses physically motivated star formation and wind prescriptions, and includes radiative transfer corrections. The models and the simulation all are found to produ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1708.07341","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1708.07341","created_at":"2026-05-18T00:36:27.730501+00:00"},{"alias_kind":"arxiv_version","alias_value":"1708.07341v1","created_at":"2026-05-18T00:36:27.730501+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1708.07341","created_at":"2026-05-18T00:36:27.730501+00:00"},{"alias_kind":"pith_short_12","alias_value":"VB3OBRRZ3NLQ","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_16","alias_value":"VB3OBRRZ3NLQI7WD","created_at":"2026-05-18T12:31:49.984773+00:00"},{"alias_kind":"pith_short_8","alias_value":"VB3OBRRZ","created_at":"2026-05-18T12:31:49.984773+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/VB3OBRRZ3NLQI7WD4BX4PTDXNM","json":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM.json","graph_json":"https://pith.science/api/pith-number/VB3OBRRZ3NLQI7WD4BX4PTDXNM/graph.json","events_json":"https://pith.science/api/pith-number/VB3OBRRZ3NLQI7WD4BX4PTDXNM/events.json","paper":"https://pith.science/paper/VB3OBRRZ"},"agent_actions":{"view_html":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM","download_json":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM.json","view_paper":"https://pith.science/paper/VB3OBRRZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1708.07341&json=true","fetch_graph":"https://pith.science/api/pith-number/VB3OBRRZ3NLQI7WD4BX4PTDXNM/graph.json","fetch_events":"https://pith.science/api/pith-number/VB3OBRRZ3NLQI7WD4BX4PTDXNM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM/action/storage_attestation","attest_author":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM/action/author_attestation","sign_citation":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM/action/citation_signature","submit_replication":"https://pith.science/pith/VB3OBRRZ3NLQI7WD4BX4PTDXNM/action/replication_record"}},"created_at":"2026-05-18T00:36:27.730501+00:00","updated_at":"2026-05-18T00:36:27.730501+00:00"}