{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:OVBIA5JG3YBWQ4ZRUSVMESAATG","short_pith_number":"pith:OVBIA5JG","schema_version":"1.0","canonical_sha256":"7542807526de03687331a4aac24800998994ef3ac9464b018480973e98846012","source":{"kind":"arxiv","id":"1205.5760","version":1},"attestation_state":"computed","paper":{"title":"A Proper Motion Study of the Haro 6-10 Outflow: Evidence for a Subarcsecond Binary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alwyn Wootten, Bradley M. Gerling, Bruce A. Wilking, Erika Gibb, Kevin B. Marvel, Mark J. Claussen","submitted_at":"2012-05-25T17:30:44Z","abstract_excerpt":"We present single-dish and VLBI observations of an outburst of water maser emission from the young binary system Haro 6-10. Haro 6-10 lies in the Taurus molecular cloud and contains a visible T Tauri star with an infrared companion 1.3\" north. Using the Very Long Baseline Array, we obtained five observations spanning 3 months and derived absolute positions for 20 distinct maser spots. Three of the masers can be traced over 3 or more epochs, enabling us to extract absolute proper motions and tangential velocities. We deduce that the masers represent one side of a bipolar outflow that lies nearl"},"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":"1205.5760","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2012-05-25T17:30:44Z","cross_cats_sorted":[],"title_canon_sha256":"30368e1d8c65d567d106353db8a6b62cc94d4542d17f60caddab7f3601fa7286","abstract_canon_sha256":"28b1b6d36394b67b4153dfab640ce296eb70fed9eb4a8c4134ce503fb3d75e6c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:57:17.129977Z","signature_b64":"DtbnCDkTSm+UkmkShKrQeA4j27hVGr5OjMPCNIfPSdrllmLlB7Si+iJ9FnPcbkxfNUJwvqF6EA6Mbd2t6GCBDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7542807526de03687331a4aac24800998994ef3ac9464b018480973e98846012","last_reissued_at":"2026-05-18T01:57:17.129547Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:57:17.129547Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Proper Motion Study of the Haro 6-10 Outflow: Evidence for a Subarcsecond Binary","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alwyn Wootten, Bradley M. Gerling, Bruce A. Wilking, Erika Gibb, Kevin B. Marvel, Mark J. Claussen","submitted_at":"2012-05-25T17:30:44Z","abstract_excerpt":"We present single-dish and VLBI observations of an outburst of water maser emission from the young binary system Haro 6-10. Haro 6-10 lies in the Taurus molecular cloud and contains a visible T Tauri star with an infrared companion 1.3\" north. Using the Very Long Baseline Array, we obtained five observations spanning 3 months and derived absolute positions for 20 distinct maser spots. Three of the masers can be traced over 3 or more epochs, enabling us to extract absolute proper motions and tangential velocities. We deduce that the masers represent one side of a bipolar outflow that lies nearl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1205.5760","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":"1205.5760","created_at":"2026-05-18T01:57:17.129611+00:00"},{"alias_kind":"arxiv_version","alias_value":"1205.5760v1","created_at":"2026-05-18T01:57:17.129611+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1205.5760","created_at":"2026-05-18T01:57:17.129611+00:00"},{"alias_kind":"pith_short_12","alias_value":"OVBIA5JG3YBW","created_at":"2026-05-18T12:27:16.716162+00:00"},{"alias_kind":"pith_short_16","alias_value":"OVBIA5JG3YBWQ4ZR","created_at":"2026-05-18T12:27:16.716162+00:00"},{"alias_kind":"pith_short_8","alias_value":"OVBIA5JG","created_at":"2026-05-18T12:27:16.716162+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/OVBIA5JG3YBWQ4ZRUSVMESAATG","json":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG.json","graph_json":"https://pith.science/api/pith-number/OVBIA5JG3YBWQ4ZRUSVMESAATG/graph.json","events_json":"https://pith.science/api/pith-number/OVBIA5JG3YBWQ4ZRUSVMESAATG/events.json","paper":"https://pith.science/paper/OVBIA5JG"},"agent_actions":{"view_html":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG","download_json":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG.json","view_paper":"https://pith.science/paper/OVBIA5JG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1205.5760&json=true","fetch_graph":"https://pith.science/api/pith-number/OVBIA5JG3YBWQ4ZRUSVMESAATG/graph.json","fetch_events":"https://pith.science/api/pith-number/OVBIA5JG3YBWQ4ZRUSVMESAATG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG/action/storage_attestation","attest_author":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG/action/author_attestation","sign_citation":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG/action/citation_signature","submit_replication":"https://pith.science/pith/OVBIA5JG3YBWQ4ZRUSVMESAATG/action/replication_record"}},"created_at":"2026-05-18T01:57:17.129611+00:00","updated_at":"2026-05-18T01:57:17.129611+00:00"}