{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:TYK7HSYTRJEGRP4ONO2FUFCEMT","short_pith_number":"pith:TYK7HSYT","schema_version":"1.0","canonical_sha256":"9e15f3cb138a4868bf8e6bb45a144464d77a10b5e12726b7d706f858112c22b7","source":{"kind":"arxiv","id":"2403.13418","version":1},"attestation_state":"computed","paper":{"title":"Constraint on magnetized galactic outflows from LOFAR rotation measure data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A.Neronov, J.Blunier","submitted_at":"2024-03-20T09:03:38Z","abstract_excerpt":"Outflows from galaxies, driven by active galactic nuclei and star formation activity, spread magnetic fields into the intergalactic medium. Importance of this process can be assessed using cosmological magneto-hydrodynamic numerical modelling of the baryonic feedback on the Large Scale Structure, like that of Illustris-TNG simulations. We use the Faraday Rotation Measure data of LOFAR Two-Meter Sky Survey (LOTSS) to test the Illustris-TNG baryonic feedback model. We show that the Illustris-TNG over-predicts the root-mean-square of the residual Rotation Measure in LOTSS. This suggests that the "},"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":"2403.13418","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-03-20T09:03:38Z","cross_cats_sorted":[],"title_canon_sha256":"2711e88d3b49af56bdba74d774dbabb99b43e7a32f48eafc5e32525be91f60cf","abstract_canon_sha256":"a0b767cf27535d44ec2b39395b6bfd6dd112400ff437e7d9b19a9c266ec3501a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:27:52.973254Z","signature_b64":"mxh//gEF9WbJez0ChlMdZTV07qwvaE7TVEKOeKX/wGLV7U3neXTTqp127MT5EbFgTTFX7mAwrn4+v+oVZePeDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9e15f3cb138a4868bf8e6bb45a144464d77a10b5e12726b7d706f858112c22b7","last_reissued_at":"2026-07-05T09:27:52.972787Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:27:52.972787Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraint on magnetized galactic outflows from LOFAR rotation measure data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A.Neronov, J.Blunier","submitted_at":"2024-03-20T09:03:38Z","abstract_excerpt":"Outflows from galaxies, driven by active galactic nuclei and star formation activity, spread magnetic fields into the intergalactic medium. Importance of this process can be assessed using cosmological magneto-hydrodynamic numerical modelling of the baryonic feedback on the Large Scale Structure, like that of Illustris-TNG simulations. We use the Faraday Rotation Measure data of LOFAR Two-Meter Sky Survey (LOTSS) to test the Illustris-TNG baryonic feedback model. We show that the Illustris-TNG over-predicts the root-mean-square of the residual Rotation Measure in LOTSS. This suggests that the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.13418","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/2403.13418/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":"2403.13418","created_at":"2026-07-05T09:27:52.972845+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.13418v1","created_at":"2026-07-05T09:27:52.972845+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.13418","created_at":"2026-07-05T09:27:52.972845+00:00"},{"alias_kind":"pith_short_12","alias_value":"TYK7HSYTRJEG","created_at":"2026-07-05T09:27:52.972845+00:00"},{"alias_kind":"pith_short_16","alias_value":"TYK7HSYTRJEGRP4O","created_at":"2026-07-05T09:27:52.972845+00:00"},{"alias_kind":"pith_short_8","alias_value":"TYK7HSYT","created_at":"2026-07-05T09:27:52.972845+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.13499","citing_title":"On the nature of LOFAR RMs and new constraints on magnetic fields in cosmic filaments and on magnetogenesis scenarios","ref_index":11,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT","json":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT.json","graph_json":"https://pith.science/api/pith-number/TYK7HSYTRJEGRP4ONO2FUFCEMT/graph.json","events_json":"https://pith.science/api/pith-number/TYK7HSYTRJEGRP4ONO2FUFCEMT/events.json","paper":"https://pith.science/paper/TYK7HSYT"},"agent_actions":{"view_html":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT","download_json":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT.json","view_paper":"https://pith.science/paper/TYK7HSYT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.13418&json=true","fetch_graph":"https://pith.science/api/pith-number/TYK7HSYTRJEGRP4ONO2FUFCEMT/graph.json","fetch_events":"https://pith.science/api/pith-number/TYK7HSYTRJEGRP4ONO2FUFCEMT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT/action/storage_attestation","attest_author":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT/action/author_attestation","sign_citation":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT/action/citation_signature","submit_replication":"https://pith.science/pith/TYK7HSYTRJEGRP4ONO2FUFCEMT/action/replication_record"}},"created_at":"2026-07-05T09:27:52.972845+00:00","updated_at":"2026-07-05T09:27:52.972845+00:00"}