{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:PIKG7L4SQNNQEMDVL3JU7QZZK7","short_pith_number":"pith:PIKG7L4S","schema_version":"1.0","canonical_sha256":"7a146faf92835b0230755ed34fc33957fea02e4742f10756a4aceb393f2971b4","source":{"kind":"arxiv","id":"1501.03681","version":1},"attestation_state":"computed","paper":{"title":"[OI]63micron jets in class 0 sources detected by Herschel","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Nisini, C. Codella, C.J. Davis, D. Neufeld, E.F. van Dishoeck, G. Herczeg, G. Santangelo, J. Eisloeffel, L. Kristensen, S. Antoniucci, S. Cabrit, T. Giannini","submitted_at":"2015-01-15T13:52:28Z","abstract_excerpt":"We present Herschel PACS mapping observations of the [OI]63 micron line towards protostellar outflows in the L1448, NGC1333-IRAS4, HH46, BHR71 and VLA1623 star forming regions. We detect emission spatially resolved along the outflow direction, which can be associated with a low excitation atomic jet. In the L1448-C, HH46 IRS and BHR71 IRS1 outflows this emission is kinematically resolved into blue- and red-shifted jet lobes, having radial velocities up to 200 km/s. In the L1448-C atomic jet the velocity increases with the distance from the protostar, similarly to what observed in the SiO jet a"},"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":"1501.03681","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2015-01-15T13:52:28Z","cross_cats_sorted":[],"title_canon_sha256":"6bf330ce47a3af52b689a794ba9aa26badd089717e924a2721eaa5741c1ce98e","abstract_canon_sha256":"57bdb113509858cac91ed35fce44040383a43c90399aa6d847890d0c734580b6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:10.814160Z","signature_b64":"Dw1pBDLcSxpnFYLh1Mxf9OTDAKsZSLbuJHbY5KefNNsFby3bb09Zz8DvM6NKKDtwyraTiYlbU59z5mnMkYZiBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7a146faf92835b0230755ed34fc33957fea02e4742f10756a4aceb393f2971b4","last_reissued_at":"2026-05-18T01:41:10.813674Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:10.813674Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"[OI]63micron jets in class 0 sources detected by Herschel","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"B. Nisini, C. Codella, C.J. Davis, D. Neufeld, E.F. van Dishoeck, G. Herczeg, G. Santangelo, J. Eisloeffel, L. Kristensen, S. Antoniucci, S. Cabrit, T. Giannini","submitted_at":"2015-01-15T13:52:28Z","abstract_excerpt":"We present Herschel PACS mapping observations of the [OI]63 micron line towards protostellar outflows in the L1448, NGC1333-IRAS4, HH46, BHR71 and VLA1623 star forming regions. We detect emission spatially resolved along the outflow direction, which can be associated with a low excitation atomic jet. In the L1448-C, HH46 IRS and BHR71 IRS1 outflows this emission is kinematically resolved into blue- and red-shifted jet lobes, having radial velocities up to 200 km/s. In the L1448-C atomic jet the velocity increases with the distance from the protostar, similarly to what observed in the SiO jet a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.03681","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":"1501.03681","created_at":"2026-05-18T01:41:10.813748+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.03681v1","created_at":"2026-05-18T01:41:10.813748+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.03681","created_at":"2026-05-18T01:41:10.813748+00:00"},{"alias_kind":"pith_short_12","alias_value":"PIKG7L4SQNNQ","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_16","alias_value":"PIKG7L4SQNNQEMDV","created_at":"2026-05-18T12:29:37.295048+00:00"},{"alias_kind":"pith_short_8","alias_value":"PIKG7L4S","created_at":"2026-05-18T12:29:37.295048+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/PIKG7L4SQNNQEMDVL3JU7QZZK7","json":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7.json","graph_json":"https://pith.science/api/pith-number/PIKG7L4SQNNQEMDVL3JU7QZZK7/graph.json","events_json":"https://pith.science/api/pith-number/PIKG7L4SQNNQEMDVL3JU7QZZK7/events.json","paper":"https://pith.science/paper/PIKG7L4S"},"agent_actions":{"view_html":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7","download_json":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7.json","view_paper":"https://pith.science/paper/PIKG7L4S","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.03681&json=true","fetch_graph":"https://pith.science/api/pith-number/PIKG7L4SQNNQEMDVL3JU7QZZK7/graph.json","fetch_events":"https://pith.science/api/pith-number/PIKG7L4SQNNQEMDVL3JU7QZZK7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7/action/storage_attestation","attest_author":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7/action/author_attestation","sign_citation":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7/action/citation_signature","submit_replication":"https://pith.science/pith/PIKG7L4SQNNQEMDVL3JU7QZZK7/action/replication_record"}},"created_at":"2026-05-18T01:41:10.813748+00:00","updated_at":"2026-05-18T01:41:10.813748+00:00"}