{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:KCO2LBUV3M4BQSRPINRZJKMGPV","short_pith_number":"pith:KCO2LBUV","schema_version":"1.0","canonical_sha256":"509da58695db38184a2f436394a9867d7aeb2a85e187a8ad230c0b8c3a26ec6e","source":{"kind":"arxiv","id":"1206.3600","version":1},"attestation_state":"computed","paper":{"title":"ALMA observations of the outflow from the Source I in the Orion-KL region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Johannes Schmid-Burgk (MPIfR), Karl M. Menten (MPIfR), Laurent Loinard (CRyA-UNAM), Luis A. Zapata (CRyA-UNAM), Luis F. Rodriguez (CRyA-UNAM), Salvador Curiel (IA-UNAM)","submitted_at":"2012-06-15T21:14:10Z","abstract_excerpt":"In this {\\it Letter}, we present sensitive millimeter SiO (J=5-4; $\\nu$=0) line observations of the outflow arising from the enigmatic object Orion Source I made with the Atacama Large Millimeter/Submillimeter Array (ALMA). The observations reveal that at scales of a few thousand AU, the outflow has a marked \"butterfly\" morphology along a northeast-southwest axis. However, contrary to what is found in the SiO and H$_2$O maser observations at scales of tens of AU, the blueshifted radial velocities of the moving gas are found to the northwest, while the redshifted velocities are in the southeast"},"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":"1206.3600","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-06-15T21:14:10Z","cross_cats_sorted":[],"title_canon_sha256":"fc3d223ff9a52f3ac854b9aefcffd927f5ec97bb8a19d96637f32e71f56a8d34","abstract_canon_sha256":"6e30544cd245ccf29f6e612469ae680c7d03c2c7a6d2723af192b4926116f31a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:52.295798Z","signature_b64":"1uiPk3OJ3GrYNfawRbkMSYFNI+XrVmFvOaQA4nL8H/IT7Kp9EBz/BM3OwN4/t7xoV+4ZOkyXB39RzzL/x+iXDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"509da58695db38184a2f436394a9867d7aeb2a85e187a8ad230c0b8c3a26ec6e","last_reissued_at":"2026-05-18T01:56:52.295189Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:52.295189Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"ALMA observations of the outflow from the Source I in the Orion-KL region","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Johannes Schmid-Burgk (MPIfR), Karl M. Menten (MPIfR), Laurent Loinard (CRyA-UNAM), Luis A. Zapata (CRyA-UNAM), Luis F. Rodriguez (CRyA-UNAM), Salvador Curiel (IA-UNAM)","submitted_at":"2012-06-15T21:14:10Z","abstract_excerpt":"In this {\\it Letter}, we present sensitive millimeter SiO (J=5-4; $\\nu$=0) line observations of the outflow arising from the enigmatic object Orion Source I made with the Atacama Large Millimeter/Submillimeter Array (ALMA). The observations reveal that at scales of a few thousand AU, the outflow has a marked \"butterfly\" morphology along a northeast-southwest axis. However, contrary to what is found in the SiO and H$_2$O maser observations at scales of tens of AU, the blueshifted radial velocities of the moving gas are found to the northwest, while the redshifted velocities are in the southeast"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.3600","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":"1206.3600","created_at":"2026-05-18T01:56:52.295265+00:00"},{"alias_kind":"arxiv_version","alias_value":"1206.3600v1","created_at":"2026-05-18T01:56:52.295265+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1206.3600","created_at":"2026-05-18T01:56:52.295265+00:00"},{"alias_kind":"pith_short_12","alias_value":"KCO2LBUV3M4B","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_16","alias_value":"KCO2LBUV3M4BQSRP","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_8","alias_value":"KCO2LBUV","created_at":"2026-05-18T12:27:11.947152+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/KCO2LBUV3M4BQSRPINRZJKMGPV","json":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV.json","graph_json":"https://pith.science/api/pith-number/KCO2LBUV3M4BQSRPINRZJKMGPV/graph.json","events_json":"https://pith.science/api/pith-number/KCO2LBUV3M4BQSRPINRZJKMGPV/events.json","paper":"https://pith.science/paper/KCO2LBUV"},"agent_actions":{"view_html":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV","download_json":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV.json","view_paper":"https://pith.science/paper/KCO2LBUV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1206.3600&json=true","fetch_graph":"https://pith.science/api/pith-number/KCO2LBUV3M4BQSRPINRZJKMGPV/graph.json","fetch_events":"https://pith.science/api/pith-number/KCO2LBUV3M4BQSRPINRZJKMGPV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV/action/storage_attestation","attest_author":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV/action/author_attestation","sign_citation":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV/action/citation_signature","submit_replication":"https://pith.science/pith/KCO2LBUV3M4BQSRPINRZJKMGPV/action/replication_record"}},"created_at":"2026-05-18T01:56:52.295265+00:00","updated_at":"2026-05-18T01:56:52.295265+00:00"}