{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:3QT4JFLFG5K2ARYAFLOGDUOIKM","short_pith_number":"pith:3QT4JFLF","schema_version":"1.0","canonical_sha256":"dc27c495653755a047002adc61d1c85303037a3d4ca34a0e0362a3ee233e6a0b","source":{"kind":"arxiv","id":"1005.1714","version":1},"attestation_state":"computed","paper":{"title":"The COMPLETE Survey of Outflows in Perseus","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alyssa A. Goodman, Hector G. Arce, Jaime E. Pineda, Michael W. Halle, Michelle A. Borkin","submitted_at":"2010-05-11T04:48:45Z","abstract_excerpt":"We present a study on the impact of molecular outflows in the Perseus molecular cloud complex using the COMPLETE survey large-scale 12CO(1-0) and 13CO(1-0) maps. We used three-dimensional isosurface models generated in RA-DEC-Velocity space to visualize the maps. This rendering of the molecular line data allowed for a rapid and efficient way to search for molecular outflows over a large (~ 16 sq. deg.) area. Our outflow-searching technique detected previously known molecular outflows as well as new candidate outflows. Most of these new outflow-related high-velocity features lie in regions that"},"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":"1005.1714","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-05-11T04:48:45Z","cross_cats_sorted":[],"title_canon_sha256":"28dc1b05c78d89577e244e5d3d5ff434fb34d47b0c3a0d8347ea4e884759f1e8","abstract_canon_sha256":"a697512061dfa11cd1a7948719d0961f4328463b307bebc8f98a4982e14a3ac0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:24:08.528562Z","signature_b64":"9z/OzaB08ZD1Lo8vqGQ/7ADuZgMMaABnVKKbtiiJPL+vxuLGgjOtxqAQBYQOWX12zycwPuCYP1bBQOfdDN6bDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dc27c495653755a047002adc61d1c85303037a3d4ca34a0e0362a3ee233e6a0b","last_reissued_at":"2026-05-18T02:24:08.527913Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:24:08.527913Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The COMPLETE Survey of Outflows in Perseus","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alyssa A. Goodman, Hector G. Arce, Jaime E. Pineda, Michael W. Halle, Michelle A. Borkin","submitted_at":"2010-05-11T04:48:45Z","abstract_excerpt":"We present a study on the impact of molecular outflows in the Perseus molecular cloud complex using the COMPLETE survey large-scale 12CO(1-0) and 13CO(1-0) maps. We used three-dimensional isosurface models generated in RA-DEC-Velocity space to visualize the maps. This rendering of the molecular line data allowed for a rapid and efficient way to search for molecular outflows over a large (~ 16 sq. deg.) area. Our outflow-searching technique detected previously known molecular outflows as well as new candidate outflows. Most of these new outflow-related high-velocity features lie in regions that"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.1714","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":"1005.1714","created_at":"2026-05-18T02:24:08.527999+00:00"},{"alias_kind":"arxiv_version","alias_value":"1005.1714v1","created_at":"2026-05-18T02:24:08.527999+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1005.1714","created_at":"2026-05-18T02:24:08.527999+00:00"},{"alias_kind":"pith_short_12","alias_value":"3QT4JFLFG5K2","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"3QT4JFLFG5K2ARYA","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"3QT4JFLF","created_at":"2026-05-18T12:26:03.138858+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.13189","citing_title":"The Accretion Process on Protostars","ref_index":178,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM","json":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM.json","graph_json":"https://pith.science/api/pith-number/3QT4JFLFG5K2ARYAFLOGDUOIKM/graph.json","events_json":"https://pith.science/api/pith-number/3QT4JFLFG5K2ARYAFLOGDUOIKM/events.json","paper":"https://pith.science/paper/3QT4JFLF"},"agent_actions":{"view_html":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM","download_json":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM.json","view_paper":"https://pith.science/paper/3QT4JFLF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1005.1714&json=true","fetch_graph":"https://pith.science/api/pith-number/3QT4JFLFG5K2ARYAFLOGDUOIKM/graph.json","fetch_events":"https://pith.science/api/pith-number/3QT4JFLFG5K2ARYAFLOGDUOIKM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM/action/storage_attestation","attest_author":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM/action/author_attestation","sign_citation":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM/action/citation_signature","submit_replication":"https://pith.science/pith/3QT4JFLFG5K2ARYAFLOGDUOIKM/action/replication_record"}},"created_at":"2026-05-18T02:24:08.527999+00:00","updated_at":"2026-05-18T02:24:08.527999+00:00"}