{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:ADGR7GXYI5YSQ66OZQWYXOZU2I","short_pith_number":"pith:ADGR7GXY","schema_version":"1.0","canonical_sha256":"00cd1f9af84771287bcecc2d8bbb34d20e46318ad6b6c39fa71a164cd055b6e1","source":{"kind":"arxiv","id":"1210.0008","version":2},"attestation_state":"computed","paper":{"title":"Discovery of an outflow of the very low-mass star ISO 143","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Pohl, T. Kopytova, V. Joergens","submitted_at":"2012-09-28T20:00:00Z","abstract_excerpt":"We discover that the very young very low-mass star ISO143 (M5) is driving an outflow based on spectro-astrometry of forbidden [SII] emission lines at 6716A and 6731A observed in UVES/VLT spectra. This adds another object to the handful of brown dwarfs and very low-mass stars (M5-M8) for which an outflow has been confirmed and which show that the T Tauri phase continues at very low masses. We find the outflow of ISO143 to be intrinsically asymmetric and the accretion disk to not obscure the outflow, as only the red outflow component is visible in the [SII] lines. ISO143 is only the third T Taur"},"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":"1210.0008","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-09-28T20:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"8ba627ad2eaab3735b6cad9fe6088bfabd357753fbcd907ef28e6f4452316bb8","abstract_canon_sha256":"7277b661f3c382ddfbb6b634486874219aba16fcc9101fc05262dfd4ec030f35"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:54:12.667246Z","signature_b64":"6UJDhQTjZeMTmZJXji5oF97+or/3v+sSIVbTqoCGdwJXovh7ZF62yOvmzc59/0pqQJpvhICISMqckMRr1ihPDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"00cd1f9af84771287bcecc2d8bbb34d20e46318ad6b6c39fa71a164cd055b6e1","last_reissued_at":"2026-05-18T01:54:12.666713Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:54:12.666713Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Discovery of an outflow of the very low-mass star ISO 143","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Pohl, T. Kopytova, V. Joergens","submitted_at":"2012-09-28T20:00:00Z","abstract_excerpt":"We discover that the very young very low-mass star ISO143 (M5) is driving an outflow based on spectro-astrometry of forbidden [SII] emission lines at 6716A and 6731A observed in UVES/VLT spectra. This adds another object to the handful of brown dwarfs and very low-mass stars (M5-M8) for which an outflow has been confirmed and which show that the T Tauri phase continues at very low masses. We find the outflow of ISO143 to be intrinsically asymmetric and the accretion disk to not obscure the outflow, as only the red outflow component is visible in the [SII] lines. ISO143 is only the third T Taur"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.0008","kind":"arxiv","version":2},"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":"1210.0008","created_at":"2026-05-18T01:54:12.666774+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.0008v2","created_at":"2026-05-18T01:54:12.666774+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.0008","created_at":"2026-05-18T01:54:12.666774+00:00"},{"alias_kind":"pith_short_12","alias_value":"ADGR7GXYI5YS","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_16","alias_value":"ADGR7GXYI5YSQ66O","created_at":"2026-05-18T12:26:58.693483+00:00"},{"alias_kind":"pith_short_8","alias_value":"ADGR7GXY","created_at":"2026-05-18T12:26:58.693483+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/ADGR7GXYI5YSQ66OZQWYXOZU2I","json":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I.json","graph_json":"https://pith.science/api/pith-number/ADGR7GXYI5YSQ66OZQWYXOZU2I/graph.json","events_json":"https://pith.science/api/pith-number/ADGR7GXYI5YSQ66OZQWYXOZU2I/events.json","paper":"https://pith.science/paper/ADGR7GXY"},"agent_actions":{"view_html":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I","download_json":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I.json","view_paper":"https://pith.science/paper/ADGR7GXY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.0008&json=true","fetch_graph":"https://pith.science/api/pith-number/ADGR7GXYI5YSQ66OZQWYXOZU2I/graph.json","fetch_events":"https://pith.science/api/pith-number/ADGR7GXYI5YSQ66OZQWYXOZU2I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I/action/storage_attestation","attest_author":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I/action/author_attestation","sign_citation":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I/action/citation_signature","submit_replication":"https://pith.science/pith/ADGR7GXYI5YSQ66OZQWYXOZU2I/action/replication_record"}},"created_at":"2026-05-18T01:54:12.666774+00:00","updated_at":"2026-05-18T01:54:12.666774+00:00"}