{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:ENGILD35JT7F7DL6WSYMINLXOI","short_pith_number":"pith:ENGILD35","schema_version":"1.0","canonical_sha256":"234c858f7d4cfe5f8d7eb4b0c43577721ba5c106dc527ddaab5f57dc9bafb306","source":{"kind":"arxiv","id":"1609.01280","version":1},"attestation_state":"computed","paper":{"title":"Molecular gas in the star-forming region IRAS 08589-4714","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"C. E. Cappa, Hugo P. Salda\\~no, J. V\\'asquez, M. G\\'omez, M. Rubio, N. U. Duronea","submitted_at":"2016-09-05T16:40:00Z","abstract_excerpt":"We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. We observed the CO(3-2), ^{13}CO(3-2), C^{18}O(3-2), HCO+(3-2), and HCN(3-2) molecular lines in a region of 150\" x 150\", centered on the IRAS source, to analyze the distribution and characteristics of the molecular gas linked to the IRAS source. The molecular gas distribution reveals a molecular clump that is coincident with IRAS 08589-4714 and with a dust clump detected at 1.2 mm. The molecular clump is 0.45 pc in radius and its mass and H_2 volume density are 310 Mo and 1.2 x 10^4 c"},"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":"1609.01280","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-09-05T16:40:00Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"e4213a32a5e85ecb93d68fec4f53cf288a88baaa335bfcebb9938daa724946b7","abstract_canon_sha256":"b78e3f6f5a37b7c84890535b66f14518661bdffbaa962e3f975a00c27f00c28c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:01:22.196936Z","signature_b64":"dc2Em25csXWTuzd/UKEV9RkfHALBBced3UJ2uCvkdfrIZEXpppMfLJP+j4gdyVijM19BpjnQPZFJOaQRWG2pAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"234c858f7d4cfe5f8d7eb4b0c43577721ba5c106dc527ddaab5f57dc9bafb306","last_reissued_at":"2026-05-18T01:01:22.196292Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:01:22.196292Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Molecular gas in the star-forming region IRAS 08589-4714","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.GA","authors_text":"C. E. Cappa, Hugo P. Salda\\~no, J. V\\'asquez, M. G\\'omez, M. Rubio, N. U. Duronea","submitted_at":"2016-09-05T16:40:00Z","abstract_excerpt":"We present an analysis of the region IRAS 08589-4714 with the aim of characterizing the molecular environment. We observed the CO(3-2), ^{13}CO(3-2), C^{18}O(3-2), HCO+(3-2), and HCN(3-2) molecular lines in a region of 150\" x 150\", centered on the IRAS source, to analyze the distribution and characteristics of the molecular gas linked to the IRAS source. The molecular gas distribution reveals a molecular clump that is coincident with IRAS 08589-4714 and with a dust clump detected at 1.2 mm. The molecular clump is 0.45 pc in radius and its mass and H_2 volume density are 310 Mo and 1.2 x 10^4 c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.01280","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":"1609.01280","created_at":"2026-05-18T01:01:22.196417+00:00"},{"alias_kind":"arxiv_version","alias_value":"1609.01280v1","created_at":"2026-05-18T01:01:22.196417+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.01280","created_at":"2026-05-18T01:01:22.196417+00:00"},{"alias_kind":"pith_short_12","alias_value":"ENGILD35JT7F","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_16","alias_value":"ENGILD35JT7F7DL6","created_at":"2026-05-18T12:30:12.583610+00:00"},{"alias_kind":"pith_short_8","alias_value":"ENGILD35","created_at":"2026-05-18T12:30:12.583610+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/ENGILD35JT7F7DL6WSYMINLXOI","json":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI.json","graph_json":"https://pith.science/api/pith-number/ENGILD35JT7F7DL6WSYMINLXOI/graph.json","events_json":"https://pith.science/api/pith-number/ENGILD35JT7F7DL6WSYMINLXOI/events.json","paper":"https://pith.science/paper/ENGILD35"},"agent_actions":{"view_html":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI","download_json":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI.json","view_paper":"https://pith.science/paper/ENGILD35","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1609.01280&json=true","fetch_graph":"https://pith.science/api/pith-number/ENGILD35JT7F7DL6WSYMINLXOI/graph.json","fetch_events":"https://pith.science/api/pith-number/ENGILD35JT7F7DL6WSYMINLXOI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI/action/storage_attestation","attest_author":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI/action/author_attestation","sign_citation":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI/action/citation_signature","submit_replication":"https://pith.science/pith/ENGILD35JT7F7DL6WSYMINLXOI/action/replication_record"}},"created_at":"2026-05-18T01:01:22.196417+00:00","updated_at":"2026-05-18T01:01:22.196417+00:00"}