{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:ORL5ACQ3FUDN6GZV63ERH3FWG2","short_pith_number":"pith:ORL5ACQ3","schema_version":"1.0","canonical_sha256":"7457d00a1b2d06df1b35f6c913ecb63680abaf0f157f8bed3935b9d8a1e88fbc","source":{"kind":"arxiv","id":"1712.07660","version":1},"attestation_state":"computed","paper":{"title":"Imaging the Molecular Outflows of the Prototypical ULIRG NGC 6240 with ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. K. Xu, D. Espada, D. Iono, H. Kaneko, J. Ueda, K. Motohara, K. Nakanishi, K. Sliwa, M. Ando, M. S. Yun, N. Lu, R. Kawabe, T. Michiyama, T. Saito, T. Yamashita","submitted_at":"2017-12-20T19:00:01Z","abstract_excerpt":"We present 0\".97 $\\times$ 0\".53 (470 pc $\\times$ 250 pc) resolution CO ($J$ = 2-1) observations toward the nearby luminous merging galaxy NGC 6240 with the Atacama Large Millimeter/submillimeter Array. We confirmed a strong CO concentration within the central 700 pc, which peaks between the double nuclei, surrounded by extended CO features along the optical dust lanes ($\\sim$11 kpc). We found that the CO emission around the central a few kpc has extremely broad velocity wings with full width at zero intensity $\\sim$ 2000 km s$^{-1}$, suggesting a possible signature of molecular outflow(s). In "},"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":"1712.07660","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-12-20T19:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"39f123616b146033ccfc42df5805a825c3b9f98635fea7bad0800f2e778ed700","abstract_canon_sha256":"3c57c747da517aa911cbb9c8ba36f759d07e7ad1b24ace2232ff441ba9bb7f59"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:23:28.307094Z","signature_b64":"BVPuoe3eFZ6sy5+sQi8OBYEhcIzGilDJx7Jz6vJhrr9kHGDnW7cCtzD1pATbkObQgSQDVIk45Y97T7iWdvHJDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7457d00a1b2d06df1b35f6c913ecb63680abaf0f157f8bed3935b9d8a1e88fbc","last_reissued_at":"2026-05-18T00:23:28.306444Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:23:28.306444Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Imaging the Molecular Outflows of the Prototypical ULIRG NGC 6240 with ALMA","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"C. K. Xu, D. Espada, D. Iono, H. Kaneko, J. Ueda, K. Motohara, K. Nakanishi, K. Sliwa, M. Ando, M. S. Yun, N. Lu, R. Kawabe, T. Michiyama, T. Saito, T. Yamashita","submitted_at":"2017-12-20T19:00:01Z","abstract_excerpt":"We present 0\".97 $\\times$ 0\".53 (470 pc $\\times$ 250 pc) resolution CO ($J$ = 2-1) observations toward the nearby luminous merging galaxy NGC 6240 with the Atacama Large Millimeter/submillimeter Array. We confirmed a strong CO concentration within the central 700 pc, which peaks between the double nuclei, surrounded by extended CO features along the optical dust lanes ($\\sim$11 kpc). We found that the CO emission around the central a few kpc has extremely broad velocity wings with full width at zero intensity $\\sim$ 2000 km s$^{-1}$, suggesting a possible signature of molecular outflow(s). In "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.07660","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":"1712.07660","created_at":"2026-05-18T00:23:28.306538+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.07660v1","created_at":"2026-05-18T00:23:28.306538+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.07660","created_at":"2026-05-18T00:23:28.306538+00:00"},{"alias_kind":"pith_short_12","alias_value":"ORL5ACQ3FUDN","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_16","alias_value":"ORL5ACQ3FUDN6GZV","created_at":"2026-05-18T12:31:34.259226+00:00"},{"alias_kind":"pith_short_8","alias_value":"ORL5ACQ3","created_at":"2026-05-18T12:31:34.259226+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/ORL5ACQ3FUDN6GZV63ERH3FWG2","json":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2.json","graph_json":"https://pith.science/api/pith-number/ORL5ACQ3FUDN6GZV63ERH3FWG2/graph.json","events_json":"https://pith.science/api/pith-number/ORL5ACQ3FUDN6GZV63ERH3FWG2/events.json","paper":"https://pith.science/paper/ORL5ACQ3"},"agent_actions":{"view_html":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2","download_json":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2.json","view_paper":"https://pith.science/paper/ORL5ACQ3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.07660&json=true","fetch_graph":"https://pith.science/api/pith-number/ORL5ACQ3FUDN6GZV63ERH3FWG2/graph.json","fetch_events":"https://pith.science/api/pith-number/ORL5ACQ3FUDN6GZV63ERH3FWG2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2/action/storage_attestation","attest_author":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2/action/author_attestation","sign_citation":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2/action/citation_signature","submit_replication":"https://pith.science/pith/ORL5ACQ3FUDN6GZV63ERH3FWG2/action/replication_record"}},"created_at":"2026-05-18T00:23:28.306538+00:00","updated_at":"2026-05-18T00:23:28.306538+00:00"}