{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:HW45KCVUJIRR7SJZBWYN7PHMAJ","short_pith_number":"pith:HW45KCVU","schema_version":"1.0","canonical_sha256":"3db9d50ab44a231fc9390db0dfbcec0240404d71cf4ac9c1979b46e0834f5f69","source":{"kind":"arxiv","id":"2504.10599","version":1},"attestation_state":"computed","paper":{"title":"Dust continuum radiation maps from MHD simulations of accretion-ejection systems around single and binary stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Christian Fendt, Sareh Ataiee, Somayeh Sheikhnezami","submitted_at":"2025-04-14T18:00:38Z","abstract_excerpt":"We study the launching of magnetized jets from a resistive circumstellar disk within a binary system, employing a unique combination of 3D MHD jet launching simulations (PLUTO code) and post-processed 3D radiative transfer modeling (RADMC-3D code). Our findings reveal a well-defined jet originating from the inner region of the disk, extending to a larger disk area. While the model attains steady states for a single star, a binary system leads to the emergence of tidal effects such as the formation of ``spiral arms'' in the disk and inside the jet. Here we have consistently implemented a time-d"},"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":"2504.10599","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-04-14T18:00:38Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"8600e4d569dd329623295c619bcd766b5f7e414373af5f4418708b838203971c","abstract_canon_sha256":"780700166a6d1decaed5214dc6e7054540223a5c1e4ac7a9aa5e4755fe9ffc60"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:49:20.391817Z","signature_b64":"9NMWzWy0E7FCZQgOQSDtq4gfx8yCyA3o6sQISJqHmGZXqtmJayGt+0MPzW+fCE6gwo0VG78RTz6tTDG3IuyoCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3db9d50ab44a231fc9390db0dfbcec0240404d71cf4ac9c1979b46e0834f5f69","last_reissued_at":"2026-07-05T10:49:20.391347Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:49:20.391347Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dust continuum radiation maps from MHD simulations of accretion-ejection systems around single and binary stars","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Christian Fendt, Sareh Ataiee, Somayeh Sheikhnezami","submitted_at":"2025-04-14T18:00:38Z","abstract_excerpt":"We study the launching of magnetized jets from a resistive circumstellar disk within a binary system, employing a unique combination of 3D MHD jet launching simulations (PLUTO code) and post-processed 3D radiative transfer modeling (RADMC-3D code). Our findings reveal a well-defined jet originating from the inner region of the disk, extending to a larger disk area. While the model attains steady states for a single star, a binary system leads to the emergence of tidal effects such as the formation of ``spiral arms'' in the disk and inside the jet. Here we have consistently implemented a time-d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.10599","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/2504.10599/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":"2504.10599","created_at":"2026-07-05T10:49:20.391407+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.10599v1","created_at":"2026-07-05T10:49:20.391407+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.10599","created_at":"2026-07-05T10:49:20.391407+00:00"},{"alias_kind":"pith_short_12","alias_value":"HW45KCVUJIRR","created_at":"2026-07-05T10:49:20.391407+00:00"},{"alias_kind":"pith_short_16","alias_value":"HW45KCVUJIRR7SJZ","created_at":"2026-07-05T10:49:20.391407+00:00"},{"alias_kind":"pith_short_8","alias_value":"HW45KCVU","created_at":"2026-07-05T10:49:20.391407+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/HW45KCVUJIRR7SJZBWYN7PHMAJ","json":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ.json","graph_json":"https://pith.science/api/pith-number/HW45KCVUJIRR7SJZBWYN7PHMAJ/graph.json","events_json":"https://pith.science/api/pith-number/HW45KCVUJIRR7SJZBWYN7PHMAJ/events.json","paper":"https://pith.science/paper/HW45KCVU"},"agent_actions":{"view_html":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ","download_json":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ.json","view_paper":"https://pith.science/paper/HW45KCVU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.10599&json=true","fetch_graph":"https://pith.science/api/pith-number/HW45KCVUJIRR7SJZBWYN7PHMAJ/graph.json","fetch_events":"https://pith.science/api/pith-number/HW45KCVUJIRR7SJZBWYN7PHMAJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ/action/storage_attestation","attest_author":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ/action/author_attestation","sign_citation":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ/action/citation_signature","submit_replication":"https://pith.science/pith/HW45KCVUJIRR7SJZBWYN7PHMAJ/action/replication_record"}},"created_at":"2026-07-05T10:49:20.391407+00:00","updated_at":"2026-07-05T10:49:20.391407+00:00"}